Circumstellar CO emission at 2.3 microns in BI Cru, He 3-1138 and He 3-1359

Details Circumstellar CO emission at 2.3 microns in BI Cru, He 3-1138 and He 3-1359 Circumstellar CO emission at 2.3 microns in BI Cru, He 3-1138 and He 3-1359

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.205.1207w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 205, Dec. 1983, p. 1207-1214.

Other

25

Carbon Monoxide, Infrared Stars, Peculiar Stars, Stellar Envelopes, Binary Stars, Mira Variables, Stellar Color, Stellar Spectra, Variable Stars

Scientific paper

Low-resolution infrared spectra of BI Cru, He 3-1138 and He 3-1359 show that these peculiar emission line stars have a 2.3 μm emission feature which the authors attribute to CO. Other data on these systems are presented. BI Cru is shown to be a symbiotic system containing a Mira variable (280 day period) but there is no evidence that He 3-1138 or He 3-1359 are symbiotics.

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