AN INTRODUCTION TO THE CHANDRA CARINA COMPLEX PROJECT
Journal Article
·
· Astrophysical Journal, Supplement Series
- Department of Astronomy and Astrophysics, 525 Davey Laboratory, Pennsylvania State University, University Park, PA 16802 (United States)
- CRESST and X-ray Astrophysics Laboratory NASA/GSFC, Greenbelt, MD 20771 (United States)
- Department of Geology and Astronomy, West Chester University, West Chester, PA 19383 (United States)
- Institut d'Astrophysique de Paris, 98bis, Bd Arago, 75014 Paris (France)
- Department of Astronomy, University of Michigan, 830 Dennison Building, Ann Arbor, MI 48109-1042 (United States)
- Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States)
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)
- GAPHE, Departement AGO, Universite de Liege, Allee du 6 Aout 17, Bat. B5C, B4000-Liege (Belgium)
- Institut d'Astrophysique et de Geophysique, Universite de Liege, 17 Allee du 6 Aout, B5c, B-4000 Sart Tilman (Belgium)
- Universitaets-Sternwarte Muenchen, Ludwig-Maximilians-Universitaet, Scheinerstr. 1, 81679 Muenchen (Germany)
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801 (United States)
The Great Nebula in Carina provides an exceptional view into the violent massive star formation and feedback that typifies giant H II regions and starburst galaxies. We have mapped the Carina star-forming complex in X-rays, using archival Chandra data and a mosaic of 20 new 60 ks pointings using the Chandra X-ray Observatory's Advanced CCD Imaging Spectrometer, as a testbed for understanding recent and ongoing star formation and to probe Carina's regions of bright diffuse X-ray emission. This study has yielded a catalog of properties of >14,000 X-ray point sources; >9800 of them have multiwavelength counterparts. Using Chandra's unsurpassed X-ray spatial resolution, we have separated these point sources from the extensive, spatially-complex diffuse emission that pervades the region; X-ray properties of this diffuse emission suggest that it traces feedback from Carina's massive stars. In this introductory paper, we motivate the survey design, describe the Chandra observations, and present some simple results, providing a foundation for the 15 papers that follow in this special issue and that present detailed catalogs, methods, and science results.
- OSTI ID:
- 21560387
- Journal Information:
- Astrophysical Journal, Supplement Series, Journal Name: Astrophysical Journal, Supplement Series Journal Issue: 1 Vol. 194; ISSN 0067-0049; ISSN APJSA2
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
79 ASTRONOMY AND ASTROPHYSICS
CATALOGS
CHARGE-COUPLED DEVICES
DOCUMENT TYPES
ELECTROMAGNETIC RADIATION
EVOLUTION
FEEDBACK
GALAXIES
IONIZING RADIATIONS
MEASURING INSTRUMENTS
NEBULAE
POINT SOURCES
RADIATION SOURCES
RADIATIONS
RESOLUTION
SEMICONDUCTOR DEVICES
SPATIAL RESOLUTION
SPECTROMETERS
STAR EVOLUTION
STARS
X RADIATION
CATALOGS
CHARGE-COUPLED DEVICES
DOCUMENT TYPES
ELECTROMAGNETIC RADIATION
EVOLUTION
FEEDBACK
GALAXIES
IONIZING RADIATIONS
MEASURING INSTRUMENTS
NEBULAE
POINT SOURCES
RADIATION SOURCES
RADIATIONS
RESOLUTION
SEMICONDUCTOR DEVICES
SPATIAL RESOLUTION
SPECTROMETERS
STAR EVOLUTION
STARS
X RADIATION