Absolute magnitude calibration for red clump stars

Karaali S., Bilir S., Gokce E. Y.

ASTROPHYSICS AND SPACE SCIENCE, cilt.346, ss.89-104, 2013 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 346
  • Basım Tarihi: 2013
  • Doi Numarası: 10.1007/s10509-013-1449-7
  • Dergi Adı: ASTROPHYSICS AND SPACE SCIENCE
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.89-104
  • İstanbul Üniversitesi Adresli: Evet

Özet

We combined the (K (s) , J-K (s) ) data in Laney et al. (Mon. Not. R. Astron. Soc. 419:1637, 2012) with the V apparent magnitudes and trigonometric parallaxes taken from the Hipparcos catalogue and used them to fit the absolute magnitude to a linear polynomial in terms of V-K (s) colour. The mean and standard deviation of the absolute magnitude residuals, -0.001 and 0.195 mag, respectively, estimated for 224 red clump stars in Laney et al. (2012) are (absolutely) smaller than the corresponding ones estimated by the procedure which adopts a mean absolute magnitude for all red clump stars, -0.053 and 0.218 mag, respectively. The statistics estimated by applying the linear equation to the data of 282 red clump stars in Alves (Astrophys. J. 539:732, 2000) are larger, and sigma=0.524 mag, which can be explained by a different absolute magnitude trend, i.e. condensation along a horizontal distribution.