The m(1)-index curve in pulsating stars

Details The m(1)-index curve in pulsating stars The m(1)-index curve in pulsating stars

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...247...77r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 247, no. 1, July 1991, p. 77-86. Research supported by Junta de Andalucia and

Astronomy and Astrophysics

Astrophysics

17

Metallicity, Stellar Oscillations, Variable Stars, Abundance, Stellar Composition

Scientific paper

We have carried out a systematic study of the behavior of the Delta-m(1) metallicity parameter for SX Phe and high amplitude Delta Sct(pop. I) stars. It is shown that it has a different behavior for the two samples of stars. The Delta-m(1) parameter increases (SX Phe) or decreases (Delta Sct) towards minimum light for these two types of variables. Moreover, the m(1)-index variation is larger when the metal abundance of the star is smaller. An analogous effect is found in, other photometric indices.

Affiliated with

Also associated with

No associations

Rating

The m(1)-index curve in pulsating stars 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 m(1)-index curve in pulsating stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The m(1)-index curve in pulsating stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-859756