Double Mode Pulsating Stars and Opacity Changes
1989 ◽
Vol 111
◽
pp. 248-248
Keyword(s):
AbstractThe basic physical properties of double mode Cepheids and double mode δ Scuti stars are still highly controversial. Based on results of very recent opacity calculations a detailed consistent, possible solution of the problem of the nature of double mode variable stars has been developed. Extensive studies have been performed to establish the rules governing the morphology of the period ratio diagrams. An ideal reproduction of the period ratio data for both stellar types are obtained assuming an increase of the Cox-Steward opacity by a factor of about 2.5 in the temperature range from 1.5 X 105K to 8.0 X 105K. Consequences for the mass calibration of Petersen diagrams are evaluated.
2002 ◽
Vol 185
◽
pp. 346-347
Keyword(s):
2019 ◽
Vol 487
(3)
◽
pp. 4457-4463
◽
Keyword(s):
2004 ◽
Vol 193
◽
pp. 279-282
Keyword(s):
2020 ◽
Vol 493
(4)
◽
pp. 5382-5388
Keyword(s):
2000 ◽
Vol 176
◽
pp. 465-466
Keyword(s):
1989 ◽
Vol 111
◽
pp. 249-249
Keyword(s):
2020 ◽
Vol 493
(3)
◽
pp. 4186-4208
◽
Keyword(s):
2015 ◽
Vol 11
(A29B)
◽
pp. 529-531
Keyword(s):