Magnetic field structure and dust distribution on CEP A

Details Magnetic field structure and dust distribution on CEP A Magnetic field structure and dust distribution on CEP A

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....97..166h&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 97, Jan. 1989, p. 166-171.

Astronomy and Astrophysics

Astronomy

8

Interstellar Magnetic Fields, Interstellar Matter, Magnetic Field Configurations, Molecular Clouds, Reflection Nebulae, Spatial Distribution, Cepheus Constellation, Interstellar Masers, Spectrum Analysis, Stellar Magnetic Fields

Scientific paper

Ice-band spectra and a high-resolution K band image of CEP A IRS 6 are presented. The spectra show indications for qualitative changes in the shape of the ice feature across the reflection nebula. The K band image shows complicated structure consisting of individual knots and filaments. H band polarization measurements of background stars behind the Cep A molecular cloud indicate a bent magnetic field in the vicinity of the Cep A star-forming region that is probably caused by interaction with the nearby Cep OB 3 association.

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