The Low Resolution Spectrum of Selected B[e] Stars with Warm Dust

Details The Low Resolution Spectrum of Selected B[e] Stars with Warm Dust The Low Resolution Spectrum of Selected B[e] Stars with Warm Dust

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..355..343p&link_type=abstract

Stars with the B[e] Phenomenon. ASP Conference Series, Vol. 355, Proceedings of the Conference Held 10-16 July, 2005, at the Isl

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We analyze the low resolution optical spectrum of several B[e] stars collected at the Loiano and Asiago Observatories within the observing campaign for hot star candidates with warm dust envelopes: IRAS 00470+6429, IRAS 01441+6026 (V 832 Cas) IRAS 06071+2925, IRAS 06070--0938 (AS 119), IRAS 07080+0605 (HBHA 717--01), IRAS 03421+2935 (MWC 728), IRAS 06259--1301 (HD 45677), and the suspected B[e] star V439 Cyg. We also observed the IRAS objects (not described here): 17449+2320, 17200-1355, 18316--0028, 19156-0935, 19587-2257, 20017+3227, and 20134+2712.

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