A critical comparison of spectroscopic and evolutionary masses for O-type binary systems

Bibcode
2003IAUS..212..216P
Penny, Laura R.; Gies, Douglas R.; Bagnuolo, William G.; Wise, John H.; Herrero, A.; Stickland, David J.; Lloyd, Chris
Referencia bibliográfica

A Massive Star Odyssey: From Main Sequence to Supernova, Proceedings of IAU Symposium #212, held 24-28 June 2001 in Lanzarote, Canary island, Spain. Edited by Karel van der Hucht, Artemio Herrero, and Esteban, César. San Francisco: Astronomical Society of the Pacific, 2003., p.216

Fecha de publicación:
2003
Número de autores
7
Número de autores del IAC
1
Número de citas
1
Número de citas referidas
0
Descripción
We have embarked on a program to directly compare spectroscopic and evolutionary masses with those obtained from a combination of spectroscopic and photometric orbital solutions for O-type binary systems. The ability to directly determine the spectroscopic masses of the individual components of O-type binary systems has been difficult, because of the severe line blending that is present in these systems. Doppler tomography is an iterative scheme, that uses an ensemble of spectra to reconstruct the individual component spectra. These individual spectra can then be analyzed.
Tipo
Sin árbitro

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