The morphology of NGC 6334 IRS V-1

Details The morphology of NGC 6334 IRS V-1 The morphology of NGC 6334 IRS V-1

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.212p..21s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 212, Jan. 1, 1985, p. 21P-25P.

Astronomy and Astrophysics

Astronomy

16

Astronomical Coordinates, Astronomical Maps, Infrared Astronomy, Nebulae, Astrometry, Morphology, Near Infrared Radiation, Reflection Nebulae

Scientific paper

High spatial resolution mapping of the region around the near-infrared source NGC 6334 IRS V-1 shows it to consist of three discrete sources, whose linear arrangement resembles a bipolar nebula. None of these sources corresponds to an object visible on the SERC I plate of this region. The high infrared polarization of the easternmost source IRS V-1 suggests that it may be a reflection nebula illuminated by a nearby hidden source, perhaps IRS V-2 or V-3.

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