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The Magnetic Field in L1457, Multiband Photopolarimetry

Show simple item record Andersson, B. en_US Wannier, P.B. en_US 2004-10-01T17:36:26Z 2004-10-01T17:36:26Z 1995 en_US
dc.identifier.citation Astrophysical Journal en_US
dc.identifier.clearanceno 95-0058 en_US
dc.description.abstract Starlight is often polarized by its passage through interstellar material. Multiband photopolarimetry towards stars behind the molecular cloud L1457 (MBM 12) has been performed. This cloud is the nearest known molecular cloud (65pc) and is thought to be contained within the local "hot bubble". The measurement of this interstellar polarization using a photopolarimeter telescope is described. en_US
dc.format.extent 802252 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other astrophysics magnetic fields stars interstellar polarization en_US
dc.title The Magnetic Field in L1457, Multiband Photopolarimetry en_US

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