The Distance to LK H α 101 Revisited

Details The Distance to LK H α 101 Revisited The Distance to LK H α 101 Revisited

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...19913401s&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #134.01; Bulletin of the American Astronomical Society, Vol. 33, p.1502

Astronomy and Astrophysics

Astronomy

Scientific paper

Lk H α 101 is a Be star with a strong ionized stellar wind and an extended H II region. The surrounding nebulosity contains many young stellar objects discovered in radio. Measurements to Lk H α 101 and its surrounding clouds have yielded distances ranging from 160 pc to 800 pc. In this poster, we discuss the various distance calculations and the physical interpretations of the objects based on it. We believe that the higher value for the distance is unrealistic, and instead believe that the objects are at a distance typical of the Taurus-Auriga cloud complex.

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