Shape of the visual light curve and detection of a 1.35 CM H2O line in single M Miras

Details Shape of the visual light curve and detection of a 1.35 CM H2O line in single M Miras Shape of the visual light curve and detection of a 1.35 CM H2O line in single M Miras

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...182...75v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 182, no. 1, Aug. 1987, p. 75-79. Research supported by the Leids Kerkhoven-Bos

Astronomy and Astrophysics

Astrophysics

10

Light Curve, Mira Variables, Stellar Spectra, Water, Centimeter Waves, Line Spectra, Stellar Envelopes

Scientific paper

The probability of detecting a 1.35 cm H2O vapor line from single M Mira variables has been found to depend on the actual shape of the visual light curve. Following the classification scheme of Ludendorff (1928), the probability of detection of H2O is highest for α-class light curves, reduces drastically for β-class, and is almost nil for γ-class. Similar tendency is exhibited by the mean luminosity of H2O in the three classes as well.

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