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CMD for atmospheres of massive stars created by using CMFGEN synthetic spectra

Published online by Cambridge University Press:  29 August 2024

Anabel Arrieta Open the ORCID record for Anabel Arrieta [Opens in a new window] ,
Agustín Payen-Sandoval ,
Lorena Arias ,
Janos Zsargo ,
Celia Fierro-Santillán  and
Jaime Klapp
Anabel Arrieta*
Affiliation:
Universidad Iberoamericana, Prolongación Paseo de la Reforma 880, Lomas de Santa Fe, 01219 Ciudad de México, México
Agustín Payen-Sandoval
Affiliation:
Universidad Iberoamericana, Prolongación Paseo de la Reforma 880, Lomas de Santa Fe, 01219 Ciudad de México, México
Lorena Arias
Affiliation:
Universidad Iberoamericana, Prolongación Paseo de la Reforma 880, Lomas de Santa Fe, 01219 Ciudad de México, México
Janos Zsargo
Affiliation:
Escuela Superior de Física y Matemáticas, IPN
Celia Fierro-Santillán
Affiliation:
ABACUS-CINESTAV
Jaime Klapp
Affiliation:
ABACUS-CINESTAV Instituto Nacional de Investigaciones Nucleares
*
email: [email protected]
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Abstract

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We present Color Magnitude Diagrams (CMDs) created by using our database of 43,340 synthetic CMFGEN spectra. For each calculated spectra we measure the absolute flux by Johnson and Gaia photometry filters and build synthetic CMDs.

Keywords

Color Magnitude Diagrammassive starHertzsprung-Russell Diagramstellar wind
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 179 - 181
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

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