CONSTRAINTS ON POROSITY AND MASS LOSS IN O-STAR WINDS FROM MODELING OF X-RAY EMISSION LINE PROFILE SHAPES (vol 770, pg 80, 2013)

被引：0
|
作者：
Leutenegger, Maurice A. [1 ,2 ,3 ]
Cohen, David H. [4 ]
Sundqvist, Jon O. [5 ,6 ]
Owocki, Stanley P. [5 ]
机构：
[1] NASA, Goddard Space Flight Ctr, CRESST, Greenbelt, MD 20771 USA
[2] NASA, Goddard Space Flight Ctr, Xray Astrophys Lab, Greenbelt, MD 20771 USA
[3] Univ Maryland Baltimore Cty, Dept Phys, Baltimore, MD 21250 USA
[4] Swarthmore Coll, Dept Phys & Astron, Swarthmore, PA 19081 USA
[5] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
[6] Univ Sternwarte Munchen, D-81679 Munich, Germany
来源：
ASTROPHYSICAL JOURNAL | 2013年 / 777卷 / 01期
关键词：
D O I：
10.1088/0004-637X/777/1/81
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页数：1
相关论文
共 19 条
  • [1] CONSTRAINTS ON POROSITY AND MASS LOSS IN O-STAR WINDS FROM THE MODELING OF X-RAY EMISSION LINE PROFILE SHAPES
    Leutenegger, Maurice A.
    Cohen, David H.
    Sundqvist, Jon O.
    Owocki, Stanley P.
    ASTROPHYSICAL JOURNAL, 2013, 770 (01):
  • [2] The x-ray emission from cloud collisions in O-star winds
    Feldmeier, A
    Pauldrach, A
    Puls, J
    BOULDER-MUNICH II: PROPERTIES OF HOT, LUMINOUS STARS, 1997, 131 : 278 - 285
  • [3] Modeling X-ray emission line profiles from massive star winds - A review
    Ignace, Richard
    ADVANCES IN SPACE RESEARCH, 2016, 58 (05) : 694 - 709
  • [4] The effect of porosity on X-ray emission-line profiles from hot-star winds
    Owocki, Stanley P.
    Cohen, David H.
    ASTROPHYSICAL JOURNAL, 2006, 648 (01): : 565 - 571
  • [5] Profile shapes for optically thick X-ray emission lines from stellar winds
    Ignace, R
    Gayley, KG
    ASTROPHYSICAL JOURNAL, 2002, 568 (02): : 954 - 964
  • [6] The X-ray emission from shock cooling zones in O star winds
    Feldmeier, A
    Kudritzki, RP
    Palsa, R
    Pauldrach, AWA
    Puls, J
    ASTRONOMY & ASTROPHYSICS, 1997, 320 (03) : 899 - 912
  • [7] Theoretical profile shapes for optically thin X-ray emission lines from spherical stellar winds
    Ignace, R
    ASTROPHYSICAL JOURNAL, 2001, 549 (01): : L119 - L123
  • [8] A generalized porosity formalism for isotropic and anisotropic effective opacity and its effects on X-ray line attenuation in clumped O star winds
    Sundqvist, Jon O.
    Owocki, Stanley P.
    Cohen, David H.
    Leutenegger, Maurice A.
    Townsend, Richard H. D.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 420 (02) : 1553 - 1561
  • [9] Mass outflow of the X-ray emission line gas in NGC 4151 (vol 493, pg 3893, 2020)
    Kraemer, S. B.
    Turner, T. J.
    Couto, J. D.
    Crenshaw, D. M.
    Schmitt, H. R.
    Revalski, M.
    Fischer, T. C.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 497 (01) : 1080 - 1080
  • [10] Extraordinarily hot X-ray emission from the O9 emission-line star HD 119682
    Rakowski, Cara E.
    Schulz, N. S.
    Wolk, S. J.
    Testa, Paola
    ASTROPHYSICAL JOURNAL, 2006, 649 (02): : L111 - L114
12