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The Herschel view of star formation in the Rosette molecular cloud under the influence of NGC 2244
Schneider, N.1; Motte, F.1; Bontemps, S.1,2; Hennemann, M.1; Di Francesco, J.3; Andre, Ph.1; Zavagno, A.4; Csengeri, T.1; Men'shchikov, A.1; Abergel, A.5; Baluteau, J. -P.4; Bernard, J. -Ph.6,7; Cox, P.8; Didelon, P.1; di Giorgio, A. -M.9; Gastaud, R.1; Griffin, M.10; Hargrave, P.10; Hill, T.1; Huang, M.11; Kirk, J.10; Koenyves, V.1; Leeks, S.12; Li, J. Z.11; Marston, A.13; Martin, P.14,15; Minier, V.1; Molinari, S.9; Olofsson, G.16; Panuzzo, P.1; Persi, P.17; Pezzuto, S.9; Roussel, H.18; Russeil, D.4; Sadavoy, S.3; Saraceno, P.9; Sauvage, M.1; Sibthorpe, B.19; Spinoglio, L.9; Testi, L.20; Teyssier, D.13; Vavrek, R.13; Ward-Thompson, D.10; White, G.12,23; Wilson, C. D.21; Woodcraft, A.22
2010-07-01
发表期刊ASTRONOMY & ASTROPHYSICS
卷号518
摘要Context. The Rosette molecular cloud is promoted as the archetype of a triggered star-formation site. This is mainly due to its morphology, because the central OB cluster NGC 2244 has blown a circular-shaped cavity into the cloud and the expanding H II-region now interacts with the cloud.
关键词Ism: Clouds Ism: General Dust Infrared: Ism Extinction Submillimeter: Ism
DOI10.1051/0004-6361/201014627
收录类别SCI
语种英语
WOS记录号WOS:000281527200084
引用统计
被引频次:32[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/7733
专题空间科学研究部
作者单位1.Univ Paris Diderot, Lab AIM, CEA DSM, INSU CNRS,IRFU SAp,CEA Saclay, F-91191 Gif Sur Yvette, France
2.Univ Bordeaux, Lab Astrophys Bordeaux, CNRS INSU, F-33271 Floirac, France
3.Univ Victoria, Dept Phys & Astron, Natl Res Council Canada, Herzberg Inst Astrophys, Victoria, BC, Canada
4.Univ Aix Marseille 1, CNRS INSU, Lab Astrophys Marseille, F-13388 Marseille 13, France
5.Univ Paris 11, IAS, F-91435 Orsay, France
6.Univ Toulouse, CESR, F-31028 Toulouse 4, France
7.Univ Toulouse, CNRS, UMR 5187, F-31028 Toulouse 4, France
8.IRAM, F-38406 St Martin Dheres, France
9.INAF IFSI, I-00133 Rome, Italy
10.Cardiff Univ, Sch Phys & Astron, Cardiff, S Glam, Wales
11.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
12.Rutherford Appleton Lab, Space Sci & Technol Dept, Didcot OX11 0QX, Oxon, England
13.ESA, Herschel Sci Ctr, ESAC, Madrid 28691, Spain
14.Univ Toronto, CITA, Toronto, ON, Canada
15.Univ Toronto, Dep Astron & Astrophys, Toronto, ON, Canada
16.Stockholm Univ, Dept Astron, AlbaNova Univ Ctr, S-10691 Stockholm, Sweden
17.INAF IASF, Sez Roma, I-00133 Rome, Italy
18.Univ Paris 06, IAP, UPMC, UMR7095, F-75014 Paris, France
19.Royal Observ, Astron Technol Ctr, Edinburgh EH9 3HJ, Midlothian, Scotland
20.ESO, D-85748 Garching, Germany
21.McMaster Univ, Dept Phys & Astron, Hamilton, ON L8S 4M1, Canada
22.Univ Edinburgh, Inst Astron, SUPA, Edinburgh EH9 3HJ, Midlothian, Scotland
23.Open Univ, Dept Phys & Astron, Milton Keynes MK7 6AA, Bucks, England
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GB/T 7714
Schneider, N.,Motte, F.,Bontemps, S.,et al. The Herschel view of star formation in the Rosette molecular cloud under the influence of NGC 2244[J]. ASTRONOMY & ASTROPHYSICS,2010,518.
APA Schneider, N..,Motte, F..,Bontemps, S..,Hennemann, M..,Di Francesco, J..,...&Woodcraft, A..(2010).The Herschel view of star formation in the Rosette molecular cloud under the influence of NGC 2244.ASTRONOMY & ASTROPHYSICS,518.
MLA Schneider, N.,et al."The Herschel view of star formation in the Rosette molecular cloud under the influence of NGC 2244".ASTRONOMY & ASTROPHYSICS 518(2010).
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