Dust formation in nova winds

被引：0
|
作者：
A. Evans
机构：
[1] Keele University,Department of Physics
来源：
Astrophysics and Space Science | 2001年 / 275卷
关键词：
Oxygen; Dust; Dust Formation; Classical Nova; Abundance Effect;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We review the properties of classical novae, with particular emphasison their dust formation. Recent observational and theoretical workindicates that CO formation in nova winds does not go to saturation,so that both oxygen- and carbon-rich condensates can appearsimultaneously in the ejected material. The UIR carrier in novaeappears to be near-unique to novae, although whether this is due toenvironmental, excitation or abundance effects is not yet clear.
引用
收藏
页码：131 / 141
页数：10
相关论文
共 50 条
  • [1] Dust formation in nova winds
    Evans, A
    ASTROPHYSICS AND SPACE SCIENCE, 2001, 275 (1-2) : 131 - 141
  • [2] DUST PROCESSING IN NOVA WINDS
    RAWLINGS, JMC
    EVANS, A
    ASTROPHYSICS AND SPACE SCIENCE, 1995, 224 (1-2) : 543 - 544
  • [3] Dust Formation in AGN Winds
    Sarangi, Arkaprabha
    Dwek, Eli
    Kazanas, Demos
    ASTROPHYSICAL JOURNAL, 2019, 885 (02):
  • [4] Nova outbursts and dust formation
    José, J
    Hernanz, M
    Amari, S
    Zinner, E
    COSMIC EVOLUTION: ON THE OCCASION OF THE 60TH BIRTHDAYS OF JEAN AUDOUZE AND JAMES W TRURAN, 2001, : 159 - 160
  • [5] DUST FORMATION IN HOT STELLAR WINDS
    CHERCHNEFF, I
    TIELENS, AGGM
    WOLF-RAYET STARS: BINARIES, COLLIDING WINDS, EVOLUTION, 1995, (163): : 346 - 354
  • [6] Dust formation and nucleosynthesis in the nova outburst
    Starrfield, S
    Gehrz, RD
    Truran, JW
    ASTROPHYSICAL IMPLICATIONS OF THE LABORATORY STUDY OF PRESOLAR MATERIALS, 1997, (402): : 203 - 234
  • [7] The Formation of Bimodal Dust Species in Nova Ejecta
    Duolikun, Adili
    Zhu, Chunhua
    Wang, Zhaojun
    Liu, Helei
    li, Lin
    Liu, Jinzhong
    Lu, Guoliang
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2019, 131 (1006)
  • [8] Dust formation in the winds of AGBs: the contribution at low metallicities
    Di Criscienzo, M.
    Dell'Agli, F.
    Ventura, P.
    Schneider, R.
    Valiante, R.
    La Franca, F.
    Rossi, C.
    Gallerani, S.
    Maiolino, R.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 433 (01) : 313 - 323
  • [9] DUST FORMATION IN STELLAR WINDS .5. THE MINIMUM MASS-LOSS RATE FOR DUST-DRIVEN WINDS
    GAIL, HP
    SEDLMAYR, E
    ASTRONOMY & ASTROPHYSICS, 1987, 177 (1-2) : 186 - 192
  • [10] Mineral formation in stellar winds - III. Dust formation in S stars
    Ferrarotti, AS
    Gail, HP
    ASTRONOMY & ASTROPHYSICS, 2002, 382 (01) : 256 - 281
12345