Chandra Orion Ultradeep Project:: Observations and source lists

被引：323

作者：

Getman, KV

Flaccomio, E

Broos, PS

Grosso, N

Tsujimoto, M

Townsley, L

Garmire, GP

Kastner, J

Li, J

Harnden, FR

Wolk, S

Murray, SS

Lada, CJ

Muench, AA

McCaughrean, MJ

Meeus, G

Damiani, F

Micela, G

Sciortino, S

Bally, J

Hillenbrand, LA

Herbst, W

Preibisch, T

Feigelson, ED

机构：

[1] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA

[2] INAF, Oservatorio Astron Palermo GS Vaiana, I-90134 Palermo, Italy

[3] Univ Grenoble 1, Lab Astrophys Grenoble, F-38041 Grenoble, France

[4] Rochester Inst Technol, Chester F Carlson Ctr Imaging Sci, Rochester, NY 14623 USA

[5] Smithsonian Astrophys Observ, Cambridge, MA 02138 USA

[6] Univ Exeter, Sch Phys, Exeter EX4 4QL, Devon, England

[7] Univ Colorado, Ctr Astrophys & Space Astron, Boulder, CO 80309 USA

[8] CALTECH, Dept Astron, Pasadena, CA 91125 USA

[9] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[10] Max Planck Inst Radioastron, D-53121 Bonn, Germany

[11] Astrophys Inst Potsdam, D-14482 Potsdam, Germany

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2005年 / 160卷 / 02期

关键词：

ISM : individual (Orion Nebula; OMC-1); open clusters and associations : individual (Orion Nebula Cluster); stars : early-type; stars : pre-main-sequence; X-rays : stars;

D O I：

10.1086/432092

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a description of the data reduction methods and the derived catalog of more than 1600 X-ray point sources from the exceptionally deep 2003 January Chandra X-Ray Observatory ( Chandra) observation of the Orion Nebula Cluster and embedded populations around OMC-1. The observation was obtained with Chandra's Advanced CCD Imaging Spectrometer (ACIS) and has been nicknamed the Chandra Orion Ultradeep Project ( COUP). With an 838 ks exposure made over a continuous period of 13.2 days, the COUP observation provides the most uniform and comprehensive data set on the X-ray emission of normal stars ever obtained in the history of X-ray astronomy.

引用

页码：319 / 352

页数：34

共 58 条

[51] X-ray modeling of very young early-type stars in the Orion Trapezium: Signatures of magnetically confined plasmas and evolutionary implications [J].