Paper:	A New Look at the Symbiotic Star RW Hydrae
Volume:	490, Stella Novae: Past and Future Decades
Page:	367
Authors:	Otulakowska-Hypka, M.; Mikolajewska, J.; Whitelock, P. A.
Abstract:	We present new estimates of the basic stellar parameters of the non-eruptive, eclipsing symbiotic system, RW Hydrae. A set of photometric and spectroscopic data was used to model this object simultaneously from the light and radial velocity curves. With new spectroscopic data we were able to improve previous results known from the literature and derive physical parameters of the system: q=4.2, M1=0.8 M⊙, M2=3.4 M⊙, R1=0.2 R⊙, R2=145 R⊙, a=350 R⊙, and i=75°.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.072 seconds