IUE observations of RCB stars during extinction minima

Details IUE observations of RCB stars during extinction minima IUE observations of RCB stars during extinction minima

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.217..767e&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 217, Dec. 15, 1985, p. 767-778.

Astronomy and Astrophysics

Astronomy

20

Cosmic Dust, R Coronae Borealis Stars, Stellar Spectra, Ultraviolet Spectra, Variable Stars, Carbon, Infrared Spectra, Light Curve, Space Observations (From Earth)

Scientific paper

The R Coronae Borealis stars RY Sgr and MV Sgr have been observed with the long-wavelength (LWR) camera on the IUE satellite during deep extinction minima. The ultraviolet spectrum of RY Sgr showed a rich chromospheric spectrum, similar to that observed in the optical spectrum of this object during previous extinction episodes. Near-simultaneous optical and near-infrared observations of MV Sgr have enabled us to deduce that the grains responsible for the extinction event in this R Coronae Borealis star had dimensions about 0.2 microns.

Affiliated with

Also associated with

No associations

Rating

IUE observations of RCB stars during extinction minima 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 IUE observations of RCB stars during extinction minima, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and IUE observations of RCB stars during extinction minima will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1163301