4.7 Article

Fundamental parameters and infrared excesses of Tycho-Gaia stars

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 471, Issue 1, Pages 770-791

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stx1433

Keywords

circumstellar matter; stars: fundamental parameters; Hertzsprung; Russell and colour; magnitude diagrams; stars: mass-loss; solar neighbourhood; infrared: stars

Funding

  1. UK Science and Technology Facility Council [ST/L000768/1]
  2. Alfred P. Sloan Foundation
  3. US Department of Energy Office of Science
  4. Center for High-Performance Computing at the University of Utah
  5. SCIENCE plan of the European Commission
  6. HCM plan of the European Commission [CT920791, CT940627]
  7. INSU in France
  8. MEN in France
  9. CNRS in France
  10. State of Baden-Wurttemberg in Germany
  11. DGICYT in Spain
  12. CNR in Italy
  13. FFwFBWF in Austria
  14. FAPESP in Brazil
  15. OTKA in Hungary [F-4239, F-013990]
  16. ESO CEE [A-04-046]
  17. National Aeronautics and Space Administration
  18. National Science Foundation
  19. Ballistic Missile Defense Organization
  20. NASA Office of Space Science
  21. ESA
  22. NASA
  23. STFC [ST/P000649/1] Funding Source: UKRI
  24. Science and Technology Facilities Council [ST/P000649/1] Funding Source: researchfish

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Effective temperatures and luminosities are calculated for 1475 921 Tycho-2 and 107 145 Hipparcos stars, based on distances from Gaia Data Release 1. Parameters are derived by comparing multi-wavelength archival photometry to BT-SETTL model atmospheres. The 1 sigma uncertainties for the Tycho-2 and Hipparcos stars are +/- 137 and +/- 125 K in temperature and +/- 35 and +/- 19 per cent in luminosity. The luminosity uncertainty is dominated by that of the Gaia parallax. Evidence for infrared excess between 4.6 and 25 mu m is found for 4256 stars, of which 1883 are strong candidates. These include asymptotic giant branch (AGB) stars, Cepheids, Herbig Ae/Be stars, young stellar objects and other sources. We briefly demonstrate the capabilities of this data set by exploring local interstellar extinction, the onset of dust production in AGB stars, the age and metallicity gradients of the solar neighbourhood and structure within the Gould Belt. We close by discussing the potential impact of future Gaia data releases.

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