4.7 Article

Fundamental parameters and infrared excesses of Hipparcos stars

期刊

出版社

WILEY-BLACKWELL
DOI: 10.1111/j.1365-2966.2012.21873.x

关键词

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

资金

  1. Alfred P. Sloan Foundation
  2. National Science Foundation
  3. U.S. Department of Energy
  4. European Commission [CT920791, CT940627]
  5. INSU
  6. MEN
  7. CNRS in France
  8. State of Baden-Wurttemberg in Germany
  9. DGICYT in Spain
  10. CNR in Italy
  11. FFwFBWF in Austria
  12. FAPESP in Brazil
  13. OTKA in Hungary [F-4239, F-013990]
  14. ESO CEE [A-04-046]
  15. National Aeronautics and Space Administration
  16. Ballistic Missile Defense Organization
  17. NASA Office of Space Science
  18. Science and Technology Facilities Council [ST/I001425/1] Funding Source: researchfish
  19. STFC [ST/I001425/1] Funding Source: UKRI

向作者/读者索取更多资源

We derive the fundamental parameters (temperature and luminosity) of 107 619 Hipparcos stars and place these stars on a true HertzsprungRussell diagram. This is achieved by comparing bt-settl model atmospheres to spectral energy distributions (SEDs) created from Hipparcos, Tycho, Sloan Digital Sky Survey, DENIS, Two Micron All Sky Survey, MSX, AKARI, IRAS and Wide-field Infrared Survey Explorer data. We also identify and quantify from these SEDs any infrared excesses attributable to circumstellar matter. We compare our results to known types of objects, focusing on the giant branch stars. Giant star dust production (as traced by infrared excess) is found to start in earnest around 680 L-circle dot.

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