An optical counterpart of the infrared bipolar nebula NGC 6334 IRS V

Details An optical counterpart of the infrared bipolar nebula NGC 6334 IRS V An optical counterpart of the infrared bipolar nebula NGC 6334 IRS V

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.228..805w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 228, Oct. 1, 1987, p. 805-809.

Astronomy and Astrophysics

Astronomy

12

Astronomical Maps, Infrared Sources (Astronomy), Nebulae

Scientific paper

The authors have discovered a faint optical counterpart of the infrared bipolar nebula NGC 6334-V. It coincides with the infrared source IRS V-2 and is strongly polarized (38 per cent). An optical polarization map in the immediate vicinity of the source indicates that IRS V-3 is the illuminating source. This, the most luminous of the four sources lying along the ridge or axis of the nebula, is very probably the origin of the bipolar outflow.

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