Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..131..479a&link_type=abstract
Astronomy and Astrophysics Supplement, v.131, p.479-482
Astronomy and Astrophysics
Astrophysics
5
Stars: Mwc 297=Iras 18250, 0351, Stars: Be, Stars: Peculiar, Stars: Variable
Scientific paper
On the basis of spectroscopic CCD material obtained at the Haute Provence Observatory, we provide line identifications and equivalent width measurements in the wavelength region 4100 - 8900 Angstroms of the spectrum of MWC 297. About two hundred features are identified, almost exclusively emission lines. Only one interstellar feature could be identified (lambda 6613) a fact which contrasts with the eigth magnitudes of extinction found by photometrists. The spectrum of the underlying star corresponds probably to a late O or early B-type object. The cooler emission lines correspond to a spectrum of a middle A-type star. Analogies with other stars observed in this series of papers are examined. Based on observations obtained at the Haute Provence Observatory (CNRS).
Andrillat Yvette
Jaschek Carlos
No associations
LandOfFree
B[e] stars. VI. MWC 297 = IRAS 18250-0351 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with B[e] stars. VI. MWC 297 = IRAS 18250-0351, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and B[e] stars. VI. MWC 297 = IRAS 18250-0351 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-810315