IRAS 1827-145P01: A possible bipolar nebula

Details IRAS 1827-145P01: A possible bipolar nebula IRAS 1827-145P01: A possible bipolar nebula

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...138..353l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 138, no. 2, Sept. 1984, p. 353-355.

Astronomy and Astrophysics

Astrophysics

9

Astronomical Photometry, Hydroxyl Emission, Infrared Spectra, Nebulae, Black Body Radiation, Interstellar Masers, Spectral Energy Distribution

Scientific paper

JHKLMN photometry of IRAS 1827-145 P01 which is the infrared counterpart of OH 17.7-2.0 is presented. The 1-100 micron energy distribution, derived from the present observations and those of IRAS, cannot be easily explained in terms of a spherically symmetric dust shell. The infrared spectrum of this source is reminiscent of a bipolar nebula (BPN). This similarity and further consideration based on OH emission data suggest that IRAS 1827-145 P01 is likely to be an OH/IR-BPN seen almost edge-on.

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