The nature of Weinberger-12

Details The nature of Weinberger-12 The nature of Weinberger-12

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97..660k&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, July 1985, p. 660-662.

Astronomy and Astrophysics

Astronomy

4

Giant Stars, Iue, Planetary Nebulae, Stellar Spectra, Subgiant Stars, Absorption Spectra, B Stars, H Alpha Line, H Ii Regions, Least Squares Method, O Stars

Scientific paper

From IUE spectra of its central star, the authors conclude that
Weinberger-12 is a small H II region, and not a planetary nebula. The
star is substantially reddened with a color excess of 0m.75,
is most likely a B0.5 - B1 giant or subgiant about three kpc distant,
and possibly belongs to the Cas OB2 association.

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