Dust in hydrogen-poor stellar winds, from theory to observations

被引：6

作者：

Cherchneff, I ^{[1
]}

机构：

[1] UMIST, Dept Phys, Manchester M60 1QD, Lancs, England

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1997年 / 251卷 / 1-2期

关键词：

SMALL CARBON CLUSTERS; WOLF-RAYET STARS; GAS-PHASE; MASS-LOSS; BUCKMINSTERFULLERENE; PHOTOMETRY; GRAPHITE; GRAINS; PLASMA; MODEL;

D O I：

10.1023/A:1000743713806

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review the nature of dust in hydrogen-deficient stellar winds, in particular cool, carbon-rich Wolf-Rayet (WC) stars, and present new observations of WC objects taken with the Short Wavelength Spectrometer on board of the ISO satellite. Predictions from theoretical models of grain precursor formation are also presented and future directions in both observational and theoretical studies are outlined.

引用

页码：333 / 342

页数：10

共 39 条

[31] STRUCTURES AND ENERGIES OF SMALL CARBON CLUSTERS - WHAT EXPERIMENT AND THEORY HAVE TO SAY ABOUT C-8(+), C-9(+) AND C-10(+) [J].

VON HELDEN, G ;

GOTTS, NG ;

PALKE, WE ;

BOWERS, MT .

INTERNATIONAL JOURNAL OF MASS SPECTROMETRY, 1994, 138 :33-47

[32] EXPERIMENTAL-EVIDENCE FOR THE FORMATION OF FULLERENES BY COLLISIONAL HEATING OF CARBON RINGS IN THE GAS-PHASE [J].

VON HELDEN, G ;

GOTTS, NG ;

BOWERS, MT .

NATURE, 1993, 363 (6424) :60-63

[33]

WILLACY K, 1997, IN PRESS A A

[34]

WILLIAMS PM, 1987, ASTRON ASTROPHYS, V182, P91

[35]

WILLIAMS PM, IN PRESS ISOS VIEW S

[36] REACTIVITY OF LARGE CARBON CLUSTERS - SPHEROIDAL CARBON SHELLS AND THEIR POSSIBLE RELEVANCE TO THE FORMATION AND MORPHOLOGY OF SOOT [J].

ZHANG, QL ;

OBRIEN, SC ;

HEATH, JR ;

LIU, Y ;

CURL, RF ;

KROTO, HW ;

SMALLEY, RE .

JOURNAL OF PHYSICAL CHEMISTRY, 1986, 90 (04) :525-528

[37]

Zubko V. G., 1992, Astronomical and Astrophysical Transactions, V3, P131, DOI 10.1080/10556799208230550

[38]

Zubko V. G., 1992, Astronomical and Astrophysical Transactions, V3, P141, DOI 10.1080/10556799208230551

[39]

ZUBKO VG, 1997, IN PRESS MNRAS

← 1 2 3 4 →