The rotating envelope of the hot star Gamma Cassiopeiae resolved by optical interferometry

Details The rotating envelope of the hot star Gamma Cassiopeiae resolved by optical interferometry The rotating envelope of the hot star Gamma Cassiopeiae resolved by optical interferometry

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989natur.342..520m&link_type=abstract

Nature (ISSN 0028-0836), vol. 342, Nov. 30, 1989, p. 520-522. Research supported by INSU.

Astronomy and Astrophysics

Astrophysics

66

B Stars, Cassiopeia Constellation, Hot Stars, Speckle Interferometry, Stellar Envelopes, Hydrogen, Roche Limit, Stellar Rotation

Scientific paper

Observations from the G12T inteferometer of the hot Be star Gamma Cassiopeiae are reported which show further high-resolution details of the hydrogen envelope. The data clearly show the envelope in rotation and approximately fit a disk model. Thus, the G12T yields optical information capable of constraining astrophysical models on the milliarcsec scale.

Affiliated with

Also associated with

No associations

Rating

The rotating envelope of the hot star Gamma Cassiopeiae resolved by optical interferometry 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 The rotating envelope of the hot star Gamma Cassiopeiae resolved by optical interferometry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The rotating envelope of the hot star Gamma Cassiopeiae resolved by optical interferometry will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1617204