The mode of pulsation in Mira variables determined by the observed acceleration data

Details The mode of pulsation in Mira variables determined by the observed acceleration data The mode of pulsation in Mira variables determined by the observed acceleration data

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...383..779t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 383, Dec. 20, 1991, p. 779-783.

Statistics

Computation

21

Mira Variables, Stellar Oscillations, Astronomical Spectroscopy, Carbon Monoxide, Computational Astrophysics, Molecular Spectra

Scientific paper

The velocity analysis, based on the observed CO molecular lines, commonly used for mode determination in Mira variables is criticized. An alternative analysis, based upon the observed acceleration and supported by new nonlinear calculations, is presented. The possibility that Mira variables are pulsating in the fundamental mode is positively rejected. The first overtone is suggested as the dominant mode of pulsation in these stars.

Affiliated with

Also associated with

No associations

Rating

The mode of pulsation in Mira variables determined by the observed acceleration data 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 mode of pulsation in Mira variables determined by the observed acceleration data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The mode of pulsation in Mira variables determined by the observed acceleration data will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1536888