UBVR sequences in M 31 and M 33

Details UBVR sequences in M 31 and M 33 UBVR sequences in M 31 and M 33

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pasp...99..380h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 99, May 1987, p. 380-386.

Astronomy and Astrophysics

Astronomy

11

Andromeda Galaxy, Astronomical Spectroscopy, Electrophotometry, Galactic Structure, Star Distribution, Ubv Spectra

Scientific paper

UBVR photoelectric photometry of sequences in two regions, M 31 and M 33, and of several transfer stars around the M 31 disk are presented and analyzed. The II and IV fields in M 31, the NE and SW fields in M 33, and the stars between 13 and 16 mag distributed around M 31 were observed with the University of Minnesota 'two-holer' photometer/polarimeter from 1982-1985. The photometric data are compared with the UBV sequences of Arp for M 31 field IV and of Sandage and Johnson (1974) for M 33. It is observed that the differences between the data are small, and therefore it is concluded that both set of data are on the same photometric system and can be used together.

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