Million-degree plasma pervading the extended Orion nebula

被引:105
作者
Guedel, Manuel [1 ,2 ,3 ,4 ,5 ]
Briggs, Kevin R. [1 ,2 ,6 ]
Montmerle, Thierry [5 ]
Audard, Marc [7 ,8 ]
Rebull, Luisa [9 ]
Skinner, Stephen L. [10 ]
机构
[1] Paul Scherrer Inst, CH-5303 Wurenlingen, Switzerland
[2] Paul Scherrer Inst, CH-5232 Villigen, Switzerland
[3] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[4] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands
[5] Univ Grenoble 1, CNRS, Lab Astrophys Grenoble, F-38041 Grenoble, France
[6] ETH, ETH Zentrum, Inst Astron, CH-8092 Zurich, Switzerland
[7] ISDC, CH-1290 Versoix, Switzerland
[8] Univ Geneva, Observ Geneva, CH-1290 Sauverny, Switzerland
[9] CALTECH, Spitzer Sci Ctr, Pasadena, CA 91125 USA
[10] Univ Colorado, Ctr Astrophys & Space Astron, Boulder, CO 80309 USA
关键词
D O I
10.1126/science.1149926
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Most stars form as members of large associations within dense, very cold ( 10 to 100 kelvin) molecular clouds. The nearby giant molecular cloud in Orion hosts several thousand stars of ages less than a few million years, many of which are located in or around the famous Orion Nebula, a prominent gas structure illuminated and ionized by a small group of massive stars ( the Trapezium). We present x- ray observations obtained with the X- ray Multi- Mirror satellite XMM- Newton, revealing that a hot plasma with a temperature of 1.7 to 2.1 million kelvin pervades the southwest extension of the nebula. The plasma flows into the adjacent interstellar medium. This x- ray outflow phenomenon must be widespread throughout our Galaxy.
引用
收藏
页码:309 / 312
页数:4
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