New Cepheid variables in the Crux-Centaurus region

Details New Cepheid variables in the Crux-Centaurus region New Cepheid variables in the Crux-Centaurus region

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978aj.....83.1390g&link_type=abstract

Astronomical Journal, vol. 83, Nov. 1978, p. 1390, 1391, 1393-1396.

Astronomy and Astrophysics

Astronomy

8

Astronomical Photography, Cepheid Variables, Galactic Structure, Milky Way Galaxy, Astrometry, Astronomical Catalogs, H Alpha Line, Photographic Plates, Position (Location), Star Distribution

Scientific paper

Two star fields in the southern Milky Way, between galactic longitudes of approximately 294 and 320 deg, have been searched for new variables. At least three long-period (periods greater than 9 days) classical Cepheids have been tentatively identified, as well as one Virginis star. The resultant distribution of Cepheids along the Milky Way in the Crux-Centaurus region indicates a concentration of spiral tracers near a longitude of about 307 deg.

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