The Magnetic Field in L1457, Multiband Photopolarimetry

Andersson, B.; Wannier, P.B.

dc.contributor.author	Andersson, B.	en_US
dc.contributor.author	Wannier, P.B.	en_US
dc.date.accessioned	2004-10-01T17:36:26Z
dc.date.available	2004-10-01T17:36:26Z
dc.date.issued	1995	en_US
dc.identifier.citation	Astrophysical Journal	en_US
dc.identifier.clearanceno	95-0058	en_US
dc.identifier.uri	http://hdl.handle.net/2014/28078
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