IRAS 01005+7910: a High Galactic Latitude Post-AGB Star

Details IRAS 01005+7910: a High Galactic Latitude Post-AGB Star IRAS 01005+7910: a High Galactic Latitude Post-AGB Star

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002chjaa...2..193h&link_type=abstract

Chinese Journal of Astronomy & Astrophysics, Vol. 2, p. 193-196

Astronomy and Astrophysics

Astrophysics

2

Stars: Post-Agb, Infrared: Stars, Stars: Evolution

Scientific paper

IRAS 01005+7910 is a cold IRAS source. We present its optical identification, photometric and spectroscopic observation results. Its optical counterpart is classified as a B2Ie star with V magnitude 10.85. Its Hα line shows the P Cygni profile. According to its location in the Galaxy (b=16.6), we consider it to be a post-AGB star or a proto-planetary nebula.

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