Physical parameters of the continuum emission layer of Mira type stars. II. Radii and expansion velocities

Details Physical parameters of the continuum emission layer of Mira type stars. II. Radii and expansion velocities Physical parameters of the continuum emission layer of Mira type stars. II. Radii and expansion velocities

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap.....50..460r&link_type=abstract

Astrophysics, Volume 50, Issue 4, pp.460-466

Astronomy and Astrophysics

Astrophysics

Stars, Spectrophotometry, Variability

Scientific paper

The Pulkovo Spectrophotometric Data Base is used to determine the
expansion velocities and radii of the continuum emission layers of the
stars RR SCO and OMICR CET. Dependences of the radii and velocities on
the phase of the variability cycle are found which agree with the known
values obtained from the layers which emit line radiation.

Affiliated with

Also associated with

No associations

Rating

Physical parameters of the continuum emission layer of Mira type stars. II. Radii and expansion velocities 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 Physical parameters of the continuum emission layer of Mira type stars. II. Radii and expansion velocities, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical parameters of the continuum emission layer of Mira type stars. II. Radii and expansion velocities will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-825200