RESONANCE LINE-PROFILES IN A-TYPE SUPER-GIANTS FROM IUE AND COPERNICUS SPECTRA

被引：0

作者：

PRADERIE, F

TALAVERA, A

LAMERS, HJGLM

机构：

[1] OBSERV PARIS, DEPT ASTROPHYS FONDAMENTALE, F-92190 MEUDON, FRANCE

[2] ASTRON INST, SPACE RES LAB, UTRECHT, NETHERLANDS

来源：

ASTRONOMY & ASTROPHYSICS | 1980年 / 86卷 / 03期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：271 / 282

页数：12

共 11 条

[1] FORMATION OF CHROMOSPHERIC RESONANCE LINE-PROFILES IN SUPER-GIANTS
BASRI, GS
ASTROPHYSICAL JOURNAL, 1980, 242 (03): : 1133 - 1143
[2] PHOTOMETRIC VARIABILITY OF B-TYPE AND A-TYPE SUPER-GIANTS
PERCY, JR
WELCH, DL
JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY OF CANADA, 1983, 77 (05) : 263 - 263
[3] PHOTOMETRIC VARIABILITY OF B-TYPE AND A-TYPE SUPER-GIANTS
PERCY, JR
WELCH, DL
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1983, 95 (570) : 491 - 505
[4] HIGHLY REDDENED M-TYPE SUPER-GIANTS FROM THE IRC CATALOG
GRASDALEN, GL
SNEDEN, C
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1979, 91 (541) : 337 - 342
[5] X-RAY LUMINOSITIES OF B SUPER-GIANTS ESTIMATED FROM ULTRAVIOLET RESONANCE LINES
ODEGARD, N
CASSINELLI, JP
ASTROPHYSICAL JOURNAL, 1982, 256 (02): : 568 - 577
[6] ROTATIONAL VELOCITIES OF LATER B-TYPE AND A-TYPE STARS AS DETERMINED FROM ULTRAVIOLET VERSUS VISUAL LINE-PROFILES
CARPENTER, KG
SLETTEBAK, A
SONNEBORN, G
ASTROPHYSICAL JOURNAL, 1984, 286 (02): : 741 - 746
[7] THE MASSES OF EARLY-TYPE STARS IN THE GALACTIC HALO DETERMINED FROM ULTRAVIOLET RESONANCE LINE-PROFILES
KEENAN, FP
DUFTON, PL
ASTRONOMY & ASTROPHYSICS, 1984, 139 (01): : 227 - 229
[8] MEASUREMENT AND MODELING OF NITROGEN RESONANCE LINE-PROFILES FROM AN ELECTRODELESS DISCHARGE LAMP
WOOD, DR
SKINNER, GB
LIFSHITZ, A
JOURNAL OF CHEMICAL PHYSICS, 1987, 87 (09): : 5092 - 5096
[9] MASS TO LINE-STRENGTH RELATIONS FROM IUE SPECTRA OF EARLY-TYPE STARS
SEKIGUCHI, K
ANDERSON, KS
ASTRONOMICAL JOURNAL, 1987, 94 (01): : 129 - 136
[10] Stellar parameters for Pop II A-type stars from IUE spectra and new-ODF ATLAS9 model atmospheres
Castelli, F
Cacciari, C
ASTRONOMY & ASTROPHYSICS, 2001, 380 (02) : 630 - 644

← 1 2 →