Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....93..833k&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 93, April 1987, p. 833-850.
Astronomy and Astrophysics
Astronomy
43
Galactic Structure, Local Group (Astronomy), Stellar Spectrophotometry, Variable Stars, Asymptotic Giant Branch Stars, Cepheid Variables, Magellanic Clouds, Stellar Evolution, Supergiant Stars
Scientific paper
A search for variable stars in M33 has been made using a series of red plates taken over a 4 yr interval from 1982 through 1985. Limiting plate magnitudes correspond to r = 21.7 mag. The total sample of variables for which periods have been determined consists of 54 long-period variables, 90 Cepheids (69 new periods), and six probable W Virginis variables. An additional 244 variables have been identified, but no regular periods have been determined. At least one of these is a Hubble-Sandage variable, but most are probably Cepheids and long-period variables. Infrared JHK photometry of a small sample of the red supergiant variables, when compared to the period-luminosity law for red supergiant variables in the Large Magellanic Cloud, yields an apparent distance modulus to M33 in K of 24.64±0.10.
Kinman Thomas D.
Mould Jeremy R.
Wood Peter R.
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