JPL Technical Report Server

The Magnetic Field in L1457, Multiband Photopolarimetry

Show simple item record

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


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account