MgII H and K line observations of Delta Scuti variables

Details MgII H and K line observations of Delta Scuti variables MgII H and K line observations of Delta Scuti variables

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...107..326f&link_type=abstract

Astronomy and Astrophysics, vol. 107, no. 2, Mar. 1982, p. 326-332. Research supported by the Consiglio Nazionale delle Ricerch

Astronomy and Astrophysics

Astrophysics

14

H Lines, K Lines, Magnesium, Spectral Line Width, Stellar Spectra, Variable Stars, Chromosphere, Iue, Scutum Constellation, Stellar Oscillations, Ultraviolet Spectra

Scientific paper

IUE observations of seven Delta Scuti variables and a comparison star are reported with a comparison of the Mg II h and k lines to those of previously observed normal stars. Evident chromospheric emission is observed in three Delta Scuti variables: tau Cyg, beta Cas and rho Pup. Possible emissions are suggested for omega-1 Eri (F2III), iota Cyg, tau Peg, and kappa-2 Boo. Values of the observed emission widths fit well in diagrams of emission width-absolute magnitude, which, if correct, confirms the suggestion by Kondo et al. (1977) of possible evidence of chromospheric emissions in late A stars. A possible relation between emission widths and periods of pulsation is also discussed.

Affiliated with

Also associated with

No associations

Rating

MgII H and K line observations of Delta Scuti variables 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 MgII H and K line observations of Delta Scuti variables, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MgII H and K line observations of Delta Scuti variables will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1014232