LkH-alpha 101 - The stellar wind, the surrounding nebula, and an associated radio star cluster

Details LkH-alpha 101 - The stellar wind, the surrounding nebula, and an associated radio star cluster LkH-alpha 101 - The stellar wind, the surrounding nebula, and an associated radio star cluster

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...324..893b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 324, Jan. 15, 1988, p. 893-898.

Astronomy and Astrophysics

Astronomy

26

H Ii Regions, Radio Sources (Astronomy), Reflection Nebulae, Star Clusters, Stellar Spectra, Stellar Winds, B Stars, Beryllium, H Alpha Line, H Beta Line, Hydrogen Masers, T Tauri Stars

Scientific paper

Radio observations of LkHα 101 have been taken to determine the characteristics of the stellar wind from the central star as well as to image the surrounding nebulosity. They also revealed the presence of a high concentration of weak compact radio sources in the neighborhood of LkHα 101, four of which have optical stellar counterparts. Spectra of three of the stars indicate two T Tauri stars and a highly obscured B star.

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