Observed and Intrinsic Properties of Binary Stars Orbits
We have analyzed the effects that the process of spectroscopic binary detection can introduce on the known statistics of these stars. Performing a Monte Carlo simulation, we have studied the possibility of having a 100% spectroscopic binarity. We show the biases in the period and mass ratio distribu...
Guardado en:
| Autores principales: | Bosch, Guillermo Luis, Meza, Amalia Margarita |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2001
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/2081 http://adsabs.harvard.edu/full/2001RMxAC..11...29B |
| Aporte de: |
Ejemplares similares
-
Gemini/GMOS search for massive binaries in the ionizing cluster of 30 DOR
por: Bosch, Guillermo, et al.
Publicado: (2009) -
Magellanic Cloud WC/WO Wolf-Rayet stars : I. Binary frequency and Roche lobe overflow formation
por: Bartzakos, P., et al.
Publicado: (2001) -
The massive Wolf-Rayet binary LSS 1964 (=WR 29)
por: Gamen, Roberto Claudio, et al.
Publicado: (2009) -
Magellanic Cloud WC/WO Wolf-Rayet stars : II. Colliding winds in binaries
por: Bartzakos, P., et al.
Publicado: (2001) -
The “Mass Discrepancy” for Massive Stars: Tests of Models Using Spectroscopic Binaries
por: Burkholder, Valorie, et al.
Publicado: (1997)