Paper:	Water Opacity in M Stars
Volume:	378, Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes
Page:	127
Authors:	Lederer, M.T.; Aringer, B.; Hoefner, S.; Kerschbaum, F.
Abstract:	We compare the recently published BT2 water line list (Barber et al. 2006) with other available lists — NASA Ames (Partridge & Schwenke 1997) and SMALL (Jørgensen et al. 2001)—and examine the impact on hydrostatic as well as dynamic models for cool M–type stars. Emerging spectra are compared to ISO–SWS observations of semiregular and Mira variables.

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 0.074 seconds