RNO 1B - A new FUor in Cassiopeia

Details RNO 1B - A new FUor in Cassiopeia RNO 1B - A new FUor in Cassiopeia

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...244l..13s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 244, no. 1, April 1991, p. L13-L16.

Astronomy and Astrophysics

Astronomy

38

Absorption Spectra, Astronomical Spectroscopy, Infrared Astronomy Satellite, Nebulae, Stellar Luminosity, Charge Coupled Devices, H Alpha Line, Herbig-Haro Objects, Stellar Composition, Stellar Structure

Scientific paper

GN 00.33.9, on the POSS red print a barely visible nebulosity within the dark cloud L 1287, is now a well defined nebula with cometary shape. The star RNO 1B, which is deeply embedded within this compact nebula, shares all properties defining a FUor: it has brightened by at least 3 mag since 1978 and its spectral type is about F8 II with a broad, variable and blueshifted P Cygni profile at H-alpha and broad, double-peaked and also variable absorption lines, including LiI 6707. The star coincides within errors with the very cold IRAS source 00338 + 6312, which drives a bipolar CO outflow.

Affiliated with

Also associated with

No associations

Rating

RNO 1B - A new FUor in Cassiopeia 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 RNO 1B - A new FUor in Cassiopeia, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and RNO 1B - A new FUor in Cassiopeia will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1787343