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?

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001assl..265..317h&link_type=abstract

Post-AGB Objects as a Phase of Stellar Evolution, Proceedings of the Toruń Workshop held July 5-7, 2000. Edited by R. Szczerba a

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

IRAS 01005+7910 is a cold IRAS source. In this paper we present the results of optical identification, photometric and spectroscopic observations. Its spectral type is classified as B2Ie, and V magnitude is 10.85. Hα shows P Cygni profile in the spectrum. According to its location in the Galaxy (b=16.6), we considered that it is a post-AGB star or a proto-planetary nebula.

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