Similarities and differences in the emission spectra of the S-type long-period variables R Andromedae and R Cygni

Details Similarities and differences in the emission spectra of the S-type long-period variables R Andromedae and R Cygni Similarities and differences in the emission spectra of the S-type long-period variables R Andromedae and R Cygni

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1536w&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Dec. 1988, p. 1536-1539.

Astronomy and Astrophysics

Astronomy

1

Emission Spectra, Stellar Spectra, Variable Stars, Line Spectra, Radial Velocity, Spectrum Analysis, Titanium, Zirconium

Scientific paper

Spectra of R Cyg obtained near the rather faint maxima of 1983 and 1984 again showed an emission spectrum characteristic of faint maxima. For R Andromedae, similar emission lines were seen in 1983 and 1984 though the maxima were actually brighter than average. An analysis of the emission lines of Ti I and Zr I seen during the 1983 cycle of R Cyg indicates an excitation temperature of 2470 K and a Zr/Ti abundance ratio enhanced over the solar ratio by 1.15 dex.

Affiliated with

Also associated with

No associations

Rating

Similarities and differences in the emission spectra of the S-type long-period variables R Andromedae and R Cygni 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 Similarities and differences in the emission spectra of the S-type long-period variables R Andromedae and R Cygni, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Similarities and differences in the emission spectra of the S-type long-period variables R Andromedae and R Cygni will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1759738