Water in K and M giant stars unveiled by ISO

Abstract

Based on the spectra obtained with Infrared Space Observatory, ISO, we detected the 6.3 micron bands of water in the late K giant Aldebaran (alpha Tau) and several early M giant stars between M0 and M3.5, which have been deemed to be too warm for tri-atomic H2O molecule to reside in their photospheres. The water column densities range 2E+17 - 2E+18 molecules/cm**2 in our sample of K and M giant stars and the excitation temperatures are 1500 K or higher. Thus, the water bands are not originating in cool stellar winds either. The presence of water in the K and early M giant stars was quite unexpected from the traditional picture of the atmosphere of the red giant star consisting of the photosphere, hot chromosphere, and cool wind. We confirm that a rather warm molecule forming region (referred to as MOLsphere) should exist as a new component of the atmosphere of red giant stars and that this should be a general phenomenon in late-type stars. ~

11 pages, 3 figures

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