Spectroscopic Study on the Atmospheric Parameters of Nearby F--K Dwarfs and Subgiants

Details Spectroscopic Study on the Atmospheric Parameters of Nearby F--K Dwarfs and Subgiants Spectroscopic Study on the Atmospheric Parameters of Nearby F--K Dwarfs and Subgiants

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pasj...57...27t&link_type=abstract

Publications of the Astronomical Society of Japan, Vol.57, No.1, pp. 27-43

Astronomy and Astrophysics

Astronomy

56

Stars: Abundances, Stars: Atmospheres, Stars: Fundamental Parameters, Stars: Late-Type

Scientific paper

Based on a collection of high-dispersion spectra obtained at Okayama Astrophysical Observatory, the atmospheric parameters (Teff, log g, vt, and [Fe/H]) of 160 mid-F through early-K stars were extensively determined by the spectroscopic method using the equivalent widths of Fe I and Fe II lines along with the numerical technique of Takeda et al. (2002, PASJ, 54, 451). The results are comprehensively discussed and compared with the parameter values derived by different approaches (e.g., photometric colors, theoretical evolutionary tracks, Hipparcos parallaxes, etc.) as well as with the published values found in various literature. It has been confirmed that our purely spectroscopic approach yields fairly reliable and consistent results.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic Study on the Atmospheric Parameters of Nearby F--K Dwarfs and Subgiants does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectroscopic Study on the Atmospheric Parameters of Nearby F--K Dwarfs and Subgiants, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic Study on the Atmospheric Parameters of Nearby F--K Dwarfs and Subgiants will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-823618