Photometric and spectroscopic observations of an unusual bipolar nebula in a BOK globule

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Photometry, Astronomical Spectroscopy, B Stars, Nebulae, Anisotropy, Bipolarity, Photosphere, Ray Tracing, Stellar Envelopes, Stellar Spectra

Scientific paper

The bipolar nebula at longitude 310 deg in the galactic plane, discovered by Bruck (1983), is a symmetrical, butterfly-shaped object whose central star is fainter in blue than the extensive lobes. The object is interpreted as a B8 star illuminating the side nebulae through gaps in a circumstellar obscuring cloud whose extinction, estimated in view of both photometric and geometrical considerations, is 3 mag. IR excess in the central star indicates a dust temperature of 780 K. The existence of the H-alpha and H-beta lines in emission in a spectrum of the central star suggests that it is surrounded by a nonisotropically radiating chromosphere whose light does not reach the side lobes. While appearing to be a newly formed star, the object is unique in being found inside an isolated Bok globule of some 50 solar masses.

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