Literature DB >> 18048651

Million-degree plasma pervading the extended Orion Nebula.

Manuel Güdel1, Kevin R Briggs, Thierry Montmerle, Marc Audard, Luisa Rebull, Stephen L Skinner.   

Abstract

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.

Entities:  

Year:  2007        PMID: 18048651     DOI: 10.1126/science.1149926

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  4 in total

1.  Waves on the surface of the Orion molecular cloud.

Authors:  Olivier Berné; Núria Marcelino; José Cernicharo
Journal:  Nature       Date:  2010-08-19       Impact factor: 49.962

2.  The first decade of science with Chandra and XMM-Newton.

Authors:  Maria Santos-Lleo; Norbert Schartel; Harvey Tananbaum; Wallace Tucker; Martin C Weisskopf
Journal:  Nature       Date:  2009-12-24       Impact factor: 49.962

3.  Disruption of the Orion molecular core 1 by wind from the massive star θ1 Orionis C.

Authors:  C Pabst; R Higgins; J R Goicoechea; D Teyssier; O Berne; E Chambers; M Wolfire; S T Suri; R Guesten; J Stutzki; U U Graf; C Risacher; A G G M Tielens
Journal:  Nature       Date:  2019-01-07       Impact factor: 49.962

4.  Expanding bubbles in Orion A: [C II] observations of M42, M43, and NGC 1977.

Authors:  C H M Pabst; J R Goicoechea; D Teyssier; O Berné; R D Higgins; E T Chambers; S Kabanovic; R Güsten; J Stutzki; A G G M Tielens
Journal:  Astron Astrophys       Date:  2020-07-01       Impact factor: 5.802

  4 in total

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