4.4 Review

Space-Based Photometry of Binary Stars: From Voyager to TESS

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Article Astronomy & Astrophysics

New eclipsing binaries with mercury-manganese stars

O. Kochukhov et al.

Summary: By studying eclipse variability in mercury-manganese (HgMn) stars, this study identifies several interesting objects requiring further investigation, including the confirmation of the longest-period eclipsing HgMn star. Additionally, eccentric systems showing heartbeat variability are reported for the first time among five newly discovered eclipsing binaries.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Massive heartbeat stars from TESS: I. TESS sectors 1-16

P. A. Kolaczek-Szymanski et al.

Summary: This study identified 20 massive heartbeat systems, with 7 exhibiting TEOs, using TESS data from the first 16 sectors and a sample of over 300 eccentric spectroscopic binaries. The results open up new possibilities for probing the interiors of massive stars and studying the interaction between pulsation and binarity in these systems.

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Tidally Excited Modes and δ Scuti Pulsations in the Eclipsing Triple Star IM Persei

Jae Woo Lee et al.

Summary: IM Per is a triple star system with accurate measurements suggesting the eclipsing components are twin dwarfs and the third light coming from a G-type tertiary companion. Analysis of the data reveals significant pulsation signals in both gravity-mode and pressure-mode regions, indicating that the pulsating component is a delta Sct variable.

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Article Astronomy & Astrophysics

TIC 168789840: A Sextuply Eclipsing Sextuple Star System

Brian P. Powell et al.

Summary: The sextuple star system TIC 168789840 is composed of three eclipsing binaries arranged in a hierarchical structure. Follow-up observations and speckle interferometry have provided insights into the system's parameters and characteristics. The system's rare composition and structure offer valuable new insights into the formation, dynamics, and evolution of multiple star systems.

ASTRONOMICAL JOURNAL (2021)

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A comparison of the dynamical and model-derived parameters of the pulsating eclipsing binary KIC 9850387

S. Sekaran et al.

Summary: By comparing the dynamical parameters and parameters derived through a combination of evolutionary and asteroseismic modeling of the pulsating eclipsing binary KIC 9850387, we aim to unravel its interior mixing profile.

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Analysis of apsidal motion in eclipsing binaries using TESS data: I. A test of gravitational theories

D. Baroch et al.

Summary: Using high-precision light curves from the TESS mission, researchers successfully determined the apsidal motion rates of multiple eclipsing binary systems and measured the general relativistic apsidal motion rates for the first time using this method. The results showed perfect agreement with theoretical predictions, allowing for stringent constraints on two parameters of the parametrised post-Newtonian formalism.

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Convective core sizes in rotating massive stars: I. Constraints from solar metallicity OB field stars

S. Martinet et al.

Summary: Spectroscopic studies of Galactic O and B stars suggest that the convective core sizes in stars more massive than about 8 solar masses at the end of the main sequence phase may be larger than predicted by stellar models. By combining stellar evolution models with spectroscopic parameters, the study examines the convective core size in massive stars and finds tensions among different methods for stars more massive than 15 solar masses.

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Spectroscopic and seismic analysis of red giants in eclipsing binaries discovered by Kepler

M. Benbakoura et al.

Summary: Eclipsing binaries are important for measuring stellar properties and constraining stellar evolution models. This study focuses on red giant stars in eclipsing binaries discovered by the NASA Kepler mission, analyzing the overestimation of mass and radius of red giants when applying asteroseismic scaling relations, the effects of close binarity on photometric modulation and oscillation suppression, and the role of tidal dissipation in binary evolution. The study also reports measurements of mass, radius, and age of M-dwarf companion stars as a by-product.

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The surface brightness-colour relations based on eclipsing binary stars and calibrated with EDR3

D. Graczyk et al.

Summary: The study aims to calibrate the surface brightness-colour relation using high-precision data from nearby eclipsing binary stars, allowing for precise predictions of angular diameters of dwarf and subgiant stars of certain spectral types.

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INTEGRAL reloaded: instruments and

Erik Kuulkers et al.

Summary: INTEGRAL, launched in 2002 by the European Space Agency, provides long, uninterrupted observations with various instruments, leading to important discoveries in astrophysics, including the detection of new high-energy sources, radioactive decay lines from supernovae, and gamma-ray polarization studies.

NEW ASTRONOMY REVIEWS (2021)

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BG Ind: the nearest doubly eclipsing, compact hierarchical quadruple system

T. Borkovits et al.

Summary: This study reveals an important discovery of a second eclipsing binary in the BG Ind system with different characteristics from the previously studied binary A. The research also confirms the stellar properties of binary A and reveals the relatively lower mass and radii of the smaller binary B.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Absolute parameters of young stars: V puppis

E. Budding et al.

Summary: New spectrometric data on V Pup combined with satellite photometry were used to revise the absolute parameters of the system, revealing insights into its evolutionary process. The system shows signs of interactive evolution and low-amplitude photometric variations, indicating a unique evolutionary path.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Evidence that short-period AM CVn systems are diverse in outburst behaviour

C. Duffy et al.

Summary: By analyzing up to 15 years of photometric data from 8 AM CVn systems, we found that they exhibit diverse long-term optical properties similar to hydrogen accreting dwarf novae. In particular, systems in the previously identified accretion disc instability region show varied behaviors resembling Z Cam systems, SU UMa systems, and nova-like systems.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

The final orbital separation in common envelope evolution

M. Politano

Summary: This paper examines the impact of adding a dynamical constraint in population synthesis calculations to explain the observed shorter orbital periods of planetary nebulae with binary cores in close binary star systems.

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Discovery and Characterization of a Rare Magnetic Hybrid β Cephei Slowly Pulsating B-type Star in an Eclipsing Binary in the Young Open Cluster NGC 6193

Keivan G. Stassun et al.

Summary: Up to 10% of OB-type stars have global magnetic fields, even though their internal structure is typically radiative. Studying these stars through eclipsing binaries and pulsations reveals interesting phenomena like hybrid beta Cep/SPB pulsators. One such discovery in the NGC 6193 cluster is HD 149834, which consists of a hybrid pulsator and a highly irradiated low-mass companion.

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TESS Observations of TX Col: Rapidly Varying Accretion Flow

Nikita Rawat et al.

Summary: By analyzing long-term photometry data, detailed periodic characteristics of the intermediate polar TX Col were studied. Changes in its accretion mechanism and the presence of quasi-periodic oscillations were observed over several days.

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Temperature and Distance Dependence of Tidal Circularization in Close Binaries: A Catalog of Eclipsing Binaries in the Southern Hemisphere Observed by the TESS Satellite

Anders B. Justesen et al.

Summary: Researchers investigate tidal circularization in close binaries using well-characterized eclipsing systems and find a clear correlation between stellar temperature, orbital separation, and eccentricities of close binaries. Some binaries with radiative envelopes may be tidally circularized more efficiently than previously assumed. These findings are important for understanding orbital circularization and have implications for explaining the observed difference in spin-orbit alignment between hot and cool host stars, especially in the context of hot Jupiters.

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BRITE observations of ν Centauri and γ Lupi, the first non-eclipsing members of the new class of nascent binaries

M. Jerzykiewicz et al.

Summary: This study reports the results of analyzing the photometry and radial-velocity observations of two single-lined spectroscopic binary systems, nu Centauri and gamma Lupi, showing that both exhibit light variations with the orbital period. The variations are caused by the reflection effect due to the heating of the secondary's hemisphere by the primary component's light. Modeling of the light curves, along with fundamental parameters of the primary components obtained from literature data, indicates that the secondary components are pre-main sequence stars transitioning onto the main sequence.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

V680 Mon - a young mercury-manganese star in an eclipsing heartbeat system

Ernst Paunzen et al.

Summary: Chemically peculiar stars in eclipsing binary systems, such as the HgMn star in the BD+09 1467 = V680 Mon system studied here, provide valuable insights into stellar parameters and evolutionary status. The system is identified as a rare `heartbeat star', with updated ephemeris and binary system parameters derived from photometric observations and modelling with the ELISA code. This fifth known eclipsing CP3 star, potentially a member of the open cluster NGC 2264, offers a unique opportunity for detailed studies and understanding of CP3 star peculiarities.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Quasi-periodic oscillations and long-term orbital period variation of the eclipsing dwarf nova EM Cyg

Wei Liu et al.

Summary: EM Cyg is an eclipsing dwarf nova with an orbital period above the period gap of cataclysmic variables. The evolution of quasi-periodic oscillations (QPOs) in EM Cyg during both outburst and quiescence was investigated based on observations. Analysis showed an increasing orbital period and characteristics of light curves during outburst, and the presence of a possible third body in the system.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Orbital and Stellar Parameters for 2M06464003+0109157: A Double-lined Eclipsing Binary of Spotted, Sub-solar Twins

Annaliese Miller et al.

Summary: This study calculated and modeled the physical and orbital properties of 2M06464003+0109157, a double lined spectroscopic binary. The analysis showed components with nearly equal masses and comparable radii, requiring the inclusion of star spots to explain eclipse variations in the light curve. The research highlights the potential for similar analyses using survey data to measure precise properties for eclipsing binaries.

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The First Photometric Investigation and Spectroscopic Analysis of Two Contact Binaries: ASAS J124343+1531.7 and LINEAR 2323566

Qiqi Xia et al.

Summary: The analysis of multi-color passband CCD light curves and TESS satellite data of two binary stars reveals different levels of magnetic activity and evolutionary states.

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC (2021)

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Quasi-periodic Oscillations in the TESS Light Curve of TX Col, a Diskless Intermediate Polar on the Precipice of Forming an Accretion Disk

Colin Littlefield et al.

Summary: The study explores different accretion modes in intermediate polars, focusing on a lesser understood mode involving a torus of diamagnetic blobs encircling the white dwarf. This mode is suggested to occur at mass-transfer rates between disk-fed and stream-fed accretion. Through analyzing the exceptional light curve of TX Col, the authors propose that the formation of a torus of diamagnetic blobs during episodes of enhanced accretion may lead to the appearance of large-amplitude quasi-periodic oscillations.

ASTRONOMICAL JOURNAL (2021)

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An all-sky sample of intermediate- to high-mass OBA-type eclipsing binaries observed by TESS

L. W. IJspeert et al.

Summary: This study aims to improve models for intermediate- to high-mass OBA-type dwarf stars by analyzing their photometric variability in eclipsing binary systems using TESS data. The research identified a large sample of potential candidates and detected 3155 unique OBA-type eclipsing binary candidates for further study of internal physical processes in this hot part of the main sequence.

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Weighing stars from birth to death: mass determination methods across the HRD

Aldo Serenelli et al.

Summary: The mass of a star is crucial for its structure, evolution, and final fate, with various methods in astronomy available to estimate or determine it. This includes both direct and model-independent approaches, as well as indirect and model-dependent methods, along with the emerging field of quantitative asteroseismology. Different evolutionary stages of stars have corresponding methods, leading to a comprehensive list of benchmark stars with recommended combination of methods for determining a "mass-ladder" for stars.

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Relations between the asteroseismic indices and stellar parameters of δ Scuti stars for two years of TESS mission

A. Hasanzadeh et al.

Summary: The study found that there is a certain scaling relationship between the asteroseismic indices and physical quantities for delta Scuti stars, with a strong positive correlation between the fundamental radial pressure mode and large frequency separation for most targets, a proportional relationship between large separation and nu(max), and a strong positive correlation between effective temperature and nu(max).

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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The EBLM project - VIII. First results for M-dwarf mass, radius, and effective temperature measurements using CHEOPS light curves

M. Swayne et al.

Summary: The accuracy of theoretical values for M-dwarf stars is debated, with discrepancies between observed and theoretical values suggesting inaccuracies towards the low-mass end of the main sequence. Using the CHEOPS satellite, high-precision light curves of eclipsing binaries are obtained to measure the mass, radius, and effective temperature of the M-dwarf stars. Initial results show consistency between CHEOPS and TESS, providing new measurements for very low-mass stars.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

The eclipsing binary systems with δ Scuti component - I. KIC10661783

A. Miszuda et al.

Summary: A comprehensive study of the eclipsing binary system KIC10661783 reveals a rich oscillation spectrum with 590 significant frequency peaks, including small-amplitude signals most likely due to gravity-mode pulsations. Binary-evolution computations show that the formation of the system was heavily influenced by rapid mass transfer, leading to instability in observed frequencies with necessary modification of mean opacity at specific temperature depths.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

HL Dra: an active Algol-like binary system with a pulsating component star and a cool third body

Xiang-dong Shi et al.

Summary: HL Draconis is an Algol-like binary system with a mass ratio of 0.361, where the secondary component exhibits strong magnetic activities. The O-C curve shows a sinusoidal variation potentially caused by the presence of a cool red dwarf third body. A total of 252 pulsation frequencies, including tidal interactions, were detected from high-precision TESS photometric data, highlighting the system's significance for further studies on binary formation, evolution, and tidal interactions.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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Space Photometry with BRITE-Constellation

Werner W. Weiss et al.

Summary: BRITE-Constellation focuses on monitoring bright stars in the Milky Way using high-precision optical photometry in red and/or blue passbands. By observing from space, it avoids the turbulent atmosphere of Earth and provides data necessary for understanding various processes inside stars. The project, a successful collaboration between Austria, Canada, and Poland, mainly studies massive and hot stars.

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V772 Cas: an ellipsoidal HgMn star in an eclipsing binary

O. Kochukhov et al.

Summary: V772 Cas is a rare example of a magnetic chemically peculiar star in an eclipsing binary system, with clear eclipses and out-of-eclipse variations. High-resolution spectroscopy reveals chemical peculiarities typical of non-magnetic HgMn stars. Modelling of the system shows that the out-of-eclipse brightness variation is explained by the ellipsoidal shape of the asynchronously rotating primary component, making it the first HgMn star with such definitively identified variability.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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A β Cephei pulsator and a changing orbital inclination in the high-mass eclipsing binary system VV Orionis

John Southworth et al.

Summary: This study analyzes the high-mass eclipsing binary system VV Ori using photometry data from the TESS satellite. The primary star shows beta Cephei pulsations while the secondary star is possibly a slowly pulsating B star. The analysis detects 51 significant oscillation frequencies, indicating tidal perturbations, and reveals that the orbital inclination is decreasing, possibly due to gravitational interactions with a third body.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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β Cephei Pulsations in the High-mass Eclipsing System CW Cephei

Jae Woo Lee et al.

Summary: CW Cep is an early B-type eclipsing binary system with precise mass measurements, showing pulsation signatures that could be orbital harmonics or secondary frequencies. These findings contribute to the asteroseismic modeling of high-mass stars.

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W. Benz et al.

Summary: CHEOPS is a small mission launched by ESA and Switzerland in December 2019 to search for transits of exoplanets using ultrahigh precision photometry on bright stars known to host planets. It aims to improve existing data and provide prime targets for future instruments to study exoplanetary atmospheres.

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Monika Lendl et al.

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TICs 167692429 and 220397947: the first compact hierarchical triple stars discovered with TESS

T. Borkovits et al.

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Unveiling the power spectra of δ Scuti stars with TESS The temperature, gravity, and frequency scaling relation

S. Barcelo Forteza et al.

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NGTS J214358.5-380102-NGTS discovery of the most eccentric known eclipsing M-dwarf binary system

Jack S. Acton et al.

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The single-sided pulsator CO Camelopardalis

D. W. Kurtz et al.

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BRITE-Constellation photometry of π5 Orionis, an ellipsoidal SPB variable

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Mixing by overshooting and rotation in intermediate-mass stars

Guglielmo Costa et al.

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ε Lupi: measuring the heartbeat of a doubly magnetic massive binary with BRITE Constellation

H. Pablo et al.

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A. Z. Bonanos et al.

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Sam Morrell et al.

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An extreme amplitude, massive heartbeat system in the LMC characterized using ASAS-SN and TESS

T. Jayasinghe et al.

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Discovery of a new WZ Sagittae-type cataclysmic variable in the Kepler/K2 data

R. Ridden-Harper et al.

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Photodynamical analysis of the triply eclipsing hierarchical triple system EPIC 249432662

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HIDES spectroscopy of bright detached eclipsing binaries from the Kepler field - III. Spectral analysis, updated parameters and new systems

K. G. Helminiak et al.

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The SDSS-HET Survey of Kepler Eclipsing Binaries. Description of the Survey and First Results

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Discovery and characterisation of long-period eclipsing binary stars from Kepler K2 campaigns 1, 2, and 3

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Discovery and characterisation of long-period eclipsing binary stars from Kepler K2 campaigns 1, 2, and 3

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Evidence for conservative mass transfer in the classical Algol system δ Librae from its surface carbon-to-nitrogen abundance ratio

A. Dervisoglu et al.

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Light-curve Instabilities of β Lyrae Observed by the BRITE Satellites

Slavek M. Rucinski et al.

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