Photometric and polarimetric observations in NGC 6334, NGC 6357 and NGC 6302.

Details Photometric and polarimetric observations in NGC 6334, NGC 6357 and NGC 6302. Photometric and polarimetric observations in NGC 6334, NGC 6357 and NGC 6302.

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979msngr..19...10n&link_type=abstract

The Messenger, vol. 19, p. 10-12

Astronomy and Astrophysics

Astronomy

1

H Ii Regions:Photometry, H Ii Regions:Polarization

Scientific paper

Polarization is observed in the light ot many stars and is normally attributed to interstellar dust particles aligned in an interstellar magnetic field. It is, however, quite possible that-at least in some cases-the polarization arises in dusty envelopes, surrounding stars during the earliest phases ot their Ide. Dr. Thorsten Neckel from the Max-Planck- Institut für Astronomie in Heidelberg, FRG, has recently obtained observations ot such objects trom La Silla. Combining photometric and polarimetric measurements, it has become possible to provide new, important evidence for the intrinsic, bipolar model.

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