NON-RADIAL PULSATIONS IN THE ZERO-AGE MAIN-SEQUENCE STAR UPSILON ORIONIS (09.5 V)

被引：7

|

作者：

SMITH, MA

机构：

[1] UNIV TEXAS,DEPT ASTRON,AUSTIN,TX 78712

[2] UNIV TEXAS,MCDONALD OBSERV,AUSTIN,TX 78712

来源：

ASTROPHYSICAL JOURNAL | 1981年 / 248卷 / 01期

关键词：

D O I：

10.1086/159145

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

收藏

页码：214 / 221

页数：8

相关论文

共 30 条

[21] STELLAR EVOLUTIONARY MODELS FROM THE ZERO-AGE MAIN-SEQUENCE TO THE 1ST THERMAL PULSE
LATTANZIO, JC
[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1991, 76 (01): : 215 - 357
[22] THE EVOLUTION OF ANGULAR-MOMENTUM AMONG ZERO-AGE MAIN-SEQUENCE SOLAR-TYPE STARS
SODERBLOM, DR
STAUFFER, JR
MACGREGOR, KB
JONES, BF
[J]. ASTROPHYSICAL JOURNAL, 1993, 409 (02): : 624 - 634
[23] Doppler imaging of two zero-age main-sequence stars in the Pleiades: HII 686 and HII 3163
Stout-Batalha, NM
Vogt, SS
[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1999, 123 (01): : 251 - 281
[24] Stellar evolution with arbitrary rotation laws. IV. Survey of zero-age main-sequence models
Deupree, RG
[J]. ASTROPHYSICAL JOURNAL, 2001, 552 (01): : 268 - 277
[25] THEORETICAL STUDIES OF MASSIVE STARS .1. EVOLUTION OF A 15M PERIOD STAR FROM ZERO-AGE MAIN-SEQUENCE TO NEON IGNITION
ENDAL, AS
[J]. ASTROPHYSICAL JOURNAL, 1975, 197 (02): : 405 - 413
[26] Core-halo structure of a chemically homogeneous massive star and bending of the zero-age main sequence
Ishii, M
Ueno, M
Kato, M
[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1999, 51 (04) : 417 - 424
[27] THE EVOLUTION OF INTERMEDIATE-MASS STARS FROM THE ZERO-AGE MAIN-SEQUENCE TO THE BASE OF THE ASYMPTOTIC GIANT BRANCH AS A FUNCTION OF MASS AND COMPOSITION
BECKER, SA
[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1981, 45 (03): : 475 - 505
[28] POSITION OF ZERO-AGE MAIN-SEQUENCE FOR STARS WITH HIGH METAL ABUNDANCE ON (MV,B-V), (MV,U-B), AND (U-B,B-V) DIAGRAMS
KHOLOPOV, PN
[J]. ASTRONOMICHESKII ZHURNAL, 1980, 57 (01): : 12 - 21
[29] The evolution of massive stars and their spectra I. A non-rotating 60 M⊙ star from the zero-age main sequence to the pre-supernova stage
Groh, Jose H.
Meynet, Georges
Ekstrom, Sylvia
Georgy, Cyril
[J]. ASTRONOMY & ASTROPHYSICS, 2014, 564
[30] STRUCTURE AND EVOLUTION OF VERY CLOSE BINARY-SYSTEMS .1. STRUCTURE EQUATIONS INCLUDING ROTATIONAL AND TIDAL DISTORTIONS AND CALCULATIONS FOR 2, 1, AND 0.65M. ZERO-AGE MAIN-SEQUENCE STARS
CHAN, KL
CHAU, WY
[J]. ASTROPHYSICAL JOURNAL, 1979, 233 (03): : 950 - 960