Related references
Note: Only part of the references are listed.Pure rotational spectra of TiO and TiO2 in VY Canis Majoris
T. Kaminski et al.
ASTRONOMY & ASTROPHYSICS (2013)
The inner wind of IRC+10216 revisited: new exotic chemistry and diagnostic for dust condensation in carbon stars
I. Cherchneff
ASTRONOMY & ASTROPHYSICS (2012)
The size, luminosity, and motion of the extreme carbon star IRC+10216 (CW Leonis)
K. M. Menten et al.
ASTRONOMY & ASTROPHYSICS (2012)
An independent distance estimate to CW Leonis
M. A. T. Groenewegen et al.
ASTRONOMY & ASTROPHYSICS (2012)
On the physical structure of IRC+10216 Ground-based and Herschel observations of CO and C2H
E. De Beck et al.
ASTRONOMY & ASTROPHYSICS (2012)
ARCSECOND RESOLUTION MAPPING OF SULFUR DIOXIDE EMISSION IN THE CIRCUMSTELLAR ENVELOPE OF VY CANIS MAJORIS
Roger R. Fu et al.
ASTROPHYSICAL JOURNAL (2012)
AN INTERFEROMETRIC SPECTRAL-LINE SURVEY OF IRC+10216 IN THE 345 GHz BAND
Nimesh A. Patel et al.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2011)
Circumstellar molecular composition of the oxygen-rich AGB star IK Tauri II. In-depth non-LTE chemical abundance analysis
L. Decin et al.
ASTRONOMY & ASTROPHYSICS (2010)
A high-resolution line survey of IRC+10216 with Herschel/HIFI First results: Detection of warm silicon dicarbide (SiC2)
J. Cernicharo et al.
ASTRONOMY & ASTROPHYSICS (2010)
Probing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles II. CO line survey of evolved stars: derivation of mass-loss rate formulae
E. De Beck et al.
ASTRONOMY & ASTROPHYSICS (2010)
COMPARATIVE SPECTRA OF OXYGEN-RICH VERSUS CARBON-RICH CIRCUMSTELLAR SHELLS: VY CANIS MAJORIS AND IRC+10216 AT 215-285 GHz
E. D. Tenenbaum et al.
ASTROPHYSICAL JOURNAL LETTERS (2010)
Circumstellar water vapour in M-type AGB stars:: radiative transfer models, abundances, and predictions for HIFI
M. Maercker et al.
ASTRONOMY & ASTROPHYSICS (2008)
Tentative detection of phosphine in IRC+10216
M. Agundez et al.
ASTRONOMY & ASTROPHYSICS (2008)
Detection of the CCP radical (X 2IIr) in IRC+10216:: A new interstellar phosphorus-containing species
D. T. Halfen et al.
ASTROPHYSICAL JOURNAL LETTERS (2008)
Constraining phosphorus chemistry in carbon- and oxygen-rich circumstellar envelopes: Observations of PN, HCP, and CP
S. N. Milam et al.
ASTROPHYSICAL JOURNAL (2008)
A spectral line survey in the 2 and 1.3 mm windows toward the carbon-rich envelope of IRC+10216
J. H. He et al.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2008)
Vibrational spectra for P4O6 and P4O10 systems:: Theoretical study from DFT quartic potential and mixed perturbation-variation method
P. Carbonniere et al.
CHEMICAL PHYSICS LETTERS (2008)
Chemical complexity in the winds of the oxygen-rich supergiant star VY Canis Majoris
L. M. Ziurys et al.
NATURE (2007)
Discovery of phosphaethyne (HCP) in space:: Phosphorus chemistry in circumstellar envelopes
Marcelino Agundez et al.
ASTROPHYSICAL JOURNAL (2007)
Identification of phosphorus monoxide (X-2 Pi(r)) in VY Canis Majoris: Detection of the first P-O bond in space
E. D. Tenenbaum et al.
ASTROPHYSICAL JOURNAL (2007)
UIR bands in the ISOSWS spectrum of the carbon star TU Tauri
C Boersma et al.
ASTRONOMY & ASTROPHYSICS (2006)
Microwave spectrum of P14N and P15N:: Spectroscopic constants and molecular structure
Gabriele Cazzoli et al.
JOURNAL OF MOLECULAR STRUCTURE (2006)
A chemical study of the inner winds of asymptotic giant branch stars
I. Cherchneff
ASTRONOMY & ASTROPHYSICS (2006)
The Cologne Database for Molecular Spectroscopy, CDMS:: a useful tool for astronomers and spectroscopists
HSP Müller et al.
JOURNAL OF MOLECULAR STRUCTURE (2005)
A rigorous attempt to verify interstellar glycine
LE Snyder et al.
ASTROPHYSICAL JOURNAL (2005)
Millimeter-wave spectroscopy of PO in excited vibrational states up to v=7
S Bailleux et al.
JOURNAL OF MOLECULAR SPECTROSCOPY (2002)
Phosphorus in circumstellar envelopes
DDS MacKay et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2001)
A λ2 mm molecular line survey of the C-star envelope IRC+10216
J Cernicharo et al.
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES (2000)
Share Paper
