Optical spectroscopy of the filamentary halo that surrounds HD 148937 and NGC 6164-65

Details Optical spectroscopy of the filamentary halo that surrounds HD 148937 and NGC 6164-65 Optical spectroscopy of the filamentary halo that surrounds HD 148937 and NGC 6164-65

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97..780f&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Sept. 1985, p. 780-783.

Astronomy and Astrophysics

Astronomy

6

Astronomical Spectroscopy, Nebulae, O Stars, Stellar Winds, Visible Spectrum, Photoionization, Shock Heating, Supernova Remnants, Ultraviolet Spectra

Scientific paper

Optical spectra have been obtained for the recently-discovered faint
filamentary halo that surrounds both the extremely young star HD 148937
and the peculiar S-shaped nebula NGC 6164-65. This halo, interpreted to
be a wind-generated interstellar bubble, has a spectrum which appears to
result from both shock-wave heating and photoionization.

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