Please use this identifier to cite or link to this item:
Title: A new discussion on the M(v) - W(O I 7774 A) relationship for F-G stars in the light of high-resolution data
Authors: Arellano Ferro, A
Giridhar, S
Goswami, A
Keywords: F stars;G stars;Oxygen spectra;Spectral line width;Stellar luminosity;Stellar spectra;B stars;Calibrating;O stars;Stellar temperature;Visible spectrum
Issue Date: May-1991
Publisher: Royal Astronomical Society
Citation: Monthly Notices of Royal Astronomical Society, Vol. 250, No.1, pp. 1 - 6
Abstract: High-resolution CCD data and a large group of F-G stars of fundamentally determined distances are used here to investigate the intrinsic nature of the M(v) - W(O I) relation and the effect of other atmospheric parameters on this relation. The M(v) - W(O I) relation is not linear in the absolute magnitude range -10 to +21. Introduction of the (b - y)0 color index to represent stellar temperature leads to a calibration of the M(v) - W(O I) - (b-y)0 relationship in the above M(v) range, which can serve as a valuable tool to determine M(v) for F-G field stars. No systematic effect of the turbulent velocity on the calibration is found.
ISSN: 0035-8711
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
goswm.pdf974.66 kBAdobe PDFView/Open

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.