Polarimetric and new photometric observations in the NGC6334/6357 region

Details Polarimetric and new photometric observations in the NGC6334/6357 region Polarimetric and new photometric observations in the NGC6334/6357 region

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...137...58n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 137, no. 1, Aug. 1984, p. 58-62.

Astronomy and Astrophysics

Astrophysics

11

Milky Way Galaxy, Molecular Clouds, O Stars, Polarimetry, Stellar Spectrophotometry, Cosmic Dust, H Ii Regions, Polarization Characteristics, Ubv Spectra

Scientific paper

UBV data for faint stars in NGC 6357 and in the dark cloud between NGC 6357 and NGC 6334 and polarization data for the brighter stars in NGC 6334 and NGC 6357 are given. 4 new O stars are identified in NGC 6357. Together with the already known O stars they can explain the excitation of the total H II region NGC 6357. The alignment of dust grains in the local spiral arm differs from the usual alignment parallel to the galactic equator by +45° and in the Sagittarius spiral arm by -45°.

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