The visible reflection nebulosity in the vicinity of Cepheus-A

Details The visible reflection nebulosity in the vicinity of Cepheus-A The visible reflection nebulosity in the vicinity of Cepheus-A

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.241..691e&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 241, Dec. 15, 1989, p. 691-696.

Astronomy and Astrophysics

Astronomy

1

Infrared Sources (Astronomy), Molecular Clouds, Optical Polarization, Reflection Nebulae, Charge Coupled Devices, Herbig-Haro Objects, Star Formation, Stellar Spectra

Scientific paper

Imaging polarization measurements are used to investigate the optical reflection nebulosity around GGD37. The two brightest reflection nebulas are illuminated by separate sources only seen in the infrared. The southern region is associated with the star forming center in Cepheus-A East, while the northern region is illuminated by a source hidden by a cometary-like dark globule.

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