Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...198l.129n&link_type=abstract
Astrophysical Journal, vol. 198, June 15, 1975, pt. 2, p. L129-L131, L133, L134. NSF-NASA-supported research.
Astronomy and Astrophysics
Astronomy
157
Infrared Astronomy, Nebulae, Stellar Evolution, Stellar Radiation, Early Stars, Late Stars, Optical Properties, Radiation Sources, Radio Astronomy
Scientific paper
Infrared, optical, and radio observation are described of a newly discovered galactic infrared source. Most of the radiation comes from a 1.''5 diameter infrared source at a temperature of about 150 K, but some visible emission in the form of a symmetrical highly polarized reflection nebulosity is also seen. The object could represent either a very early or a very late stage in stellar evolution.
Becklin Eric E.
Merrill Michael K.
Neugebauer Gernot
Ney Peter E.
Wynn-Williams C. G.
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