A CATALOG OF CHANDRA X-RAY SOURCES IN THE CARINA NEBULA

被引：82

作者：

Broos, Patrick S. ^{[1
]}

Townsley, Leisa K. ^{[1
]}

Feigelson, Eric D. ^{[1
]}

Getman, Konstantin V. ^{[1
]}

Garmire, Gordon P. ^{[1
]}

Preibisch, Thomas ^{[2
]}

Smith, Nathan ^{[3
]}

Babler, Brian L. ^{[4
]}

Hodgkin, Simon ^{[5
]}

Indebetouw, Remy ^{[6
]}

Irwin, Mike ^{[5
]}

King, Robert R. ^{[7
]}

Lewis, Jim ^{[5
]}

Majewski, Steven R. ^{[6
]}

McCaughrean, Mark J. ^{[7
,8
]}

Meade, Marilyn R. ^{[4
]}

Zinnecker, Hans ^{[9
]}

机构：

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

[2] Univ Munich, Univ Sternwarte, D-81679 Munich, Germany

[3] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA

[4] Univ Wisconsin, Dept Astron, Madison, WI 53706 USA

[5] Inst Astron, Cambridge Astron Survey Unit, Cambridge CB3, England

[6] Univ Virginia, Dept Astron, Charlottesville, VA 22904 USA

[7] Univ Exeter, Astrophys Grp, Coll Engn Math & Phys Sci, Exeter EX4 4QL, Devon, England

[8] European Space Agcy, Res & Sci Support Dept, Estec, NL-2200 AG Noordwijk, Netherlands

[9] Astrophy Inst Potsdam, D-14482 Potsdam, Germany

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2011年 / 194卷 / 01期

基金：

美国国家航空航天局; 美国国家科学基金会;

关键词：

ISM: individual objects (Carina Nebula); open clusters and associations: individual (Tr14; Tr15; Tr16); stars: formation; stars: pre-main sequence; X-rays: stars; CCD IMAGING SPECTROMETER; CHARGE-TRANSFER INEFFICIENCY; SKY SURVEY 2MASS; PROPER MOTIONS; STAR-FORMATION; OPEN CLUSTERS; ETA-CARINAE; TRUMPLER; 14; ACIS; PHOTOMETRY;

D O I：

10.1088/0067-0049/194/1/2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a catalog of similar to 14,000 X-ray sources observed by the ACIS instrument on the Chandra X-ray Observatory within a 1.42 deg(2) survey of the Great Nebula in Carina, known as the Chandra Carina Complex Project ( CCCP). This study appears in a special issue devoted to the CCCP. Here, we describe the data reduction and analysis procedures performed on the X-ray observations, including calibration and cleaning of the X-ray event data, point-source detection, and source extraction. The catalog appears to be complete across most of the field to an absorption-corrected total-band luminosity of similar to 10(30.7) erg s(-1) for a typical low-mass pre-main-sequence star. Counterparts to the X-ray sources are identified in a variety of visual, near-infrared, and mid-infrared surveys. The X-ray and infrared source properties presented here form the basis of many CCCP studies of the young stellar populations in Carina.

引用

页数：19

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