Semi-analytical Formulas for the Hertzsprung-Russell Diagram

The absolute visual magnitude as function of the observed color (B-V), also named Hertzsprung-Russell diagram, can be described through five equations; that when calibrated stars are available means eight constants. The developed framework allows to deduce the remaining physical parameters, mass, r...

Full description

Bibliographic Details
Main Author: Zaninetti, L.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2008-12-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://saj.matf.bg.ac.rs/177/pdf/073-085.pdf
_version_ 1818751984466919424
author Zaninetti, L.
author_facet Zaninetti, L.
author_sort Zaninetti, L.
collection DOAJ
description The absolute visual magnitude as function of the observed color (B-V), also named Hertzsprung-Russell diagram, can be described through five equations; that when calibrated stars are available means eight constants. The developed framework allows to deduce the remaining physical parameters, mass, radius and luminosity. This new technique is applied to the first 10 pc, the first 50 pc, the Hyades and to the determination of the distance of a cluster. The case of the white dwarfs is analyzed assuming the absence of calibrated data: our equation produces a smaller $chi^2$ with respect to the standard color-magnitude calibration when applied to the Villanova Catalog of Spectroscopically Identified White Dwarfs. The theoretical basis of the formulas for the colors and the bolometric correction of the stars is clarified by a Taylor expansion in the temperature of the Planck distribution.
first_indexed 2024-12-18T04:44:15Z
format Article
id doaj.art-fecf88eb9cb343b78bf03853ba3961f8
institution Directory Open Access Journal
issn 1450-698X
language English
last_indexed 2024-12-18T04:44:15Z
publishDate 2008-12-01
publisher Astronomical Observatory, Department of Astronomy, Belgrade
record_format Article
series Serbian Astronomical Journal
spelling doaj.art-fecf88eb9cb343b78bf03853ba3961f82022-12-21T21:20:38ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X2008-12-011777385Semi-analytical Formulas for the Hertzsprung-Russell DiagramZaninetti, L.The absolute visual magnitude as function of the observed color (B-V), also named Hertzsprung-Russell diagram, can be described through five equations; that when calibrated stars are available means eight constants. The developed framework allows to deduce the remaining physical parameters, mass, radius and luminosity. This new technique is applied to the first 10 pc, the first 50 pc, the Hyades and to the determination of the distance of a cluster. The case of the white dwarfs is analyzed assuming the absence of calibrated data: our equation produces a smaller $chi^2$ with respect to the standard color-magnitude calibration when applied to the Villanova Catalog of Spectroscopically Identified White Dwarfs. The theoretical basis of the formulas for the colors and the bolometric correction of the stars is clarified by a Taylor expansion in the temperature of the Planck distribution.http://saj.matf.bg.ac.rs/177/pdf/073-085.pdfStars: fundamental parametersHertzsprung-Russell (HR) and C-MStars: general
spellingShingle Zaninetti, L.
Semi-analytical Formulas for the Hertzsprung-Russell Diagram
Serbian Astronomical Journal
Stars: fundamental parameters
Hertzsprung-Russell (HR) and C-M
Stars: general
title Semi-analytical Formulas for the Hertzsprung-Russell Diagram
title_full Semi-analytical Formulas for the Hertzsprung-Russell Diagram
title_fullStr Semi-analytical Formulas for the Hertzsprung-Russell Diagram
title_full_unstemmed Semi-analytical Formulas for the Hertzsprung-Russell Diagram
title_short Semi-analytical Formulas for the Hertzsprung-Russell Diagram
title_sort semi analytical formulas for the hertzsprung russell diagram
topic Stars: fundamental parameters
Hertzsprung-Russell (HR) and C-M
Stars: general
url http://saj.matf.bg.ac.rs/177/pdf/073-085.pdf
work_keys_str_mv AT zaninettil semianalyticalformulasforthehertzsprungrusselldiagram