The illumination of the cometary nebula 1548C27

Details The illumination of the cometary nebula 1548C27 The illumination of the cometary nebula 1548C27

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.249..310s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 249, March 15, 1991, p. 310-312. SERC-supported researc

Other

8

Early Stars, Illuminating, Reflection Nebulae, Charge Coupled Devices, Emission Spectra, Molecular Flow, Optical Polarization

Scientific paper

A polarization map of the 1548C27 nebulosity indicates that, in addition to the star at the geometric center of the nebulosity, there is another star about 10 arcsec to the northeast which also illuminates the nebulosity and the inner part of the jet. This finding indicates that either star could be the origin of the jet feature. If it is confirmed that this second source is a YSO, then this would represent another example of the Haro 6-5 phenomenon in which two nearby young stars are involved in illuminating contiguous nebulosity associated with a jet feature.

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