An X-ray View of Star Formation in the Central 3 kpc of NGC 2403
arXiv:0912.5135 · doi:10.1088/0004-6256/139/3/1066
Abstract
Archival Chandra observations are used to study the X-ray emission associated with star formation in the central region of the nearby SAB(s)cd galaxy NGC 2403. The distribution of X-ray emission is compared to the morphology visible at other wavelengths using complementary Spitzer, GALEX, and ground-based Halpha imagery. In general, the brightest extended X-ray emission is associated with HII regions and to other star-forming structures but is more pervasive; existing also in regions devoid of strong Halpha and UV emission. This X-ray emission has the spectral properties of diffuse hot gas (kT ~ 0.2keV) whose likely origin is in gas shock-heated by stellar winds and supernovae with < 20% coming from faint unresolved X-ray point sources. This hot gas may be slowly-cooling extra-planar remnants of past outflow events, or a disk component that either lingers after local star formation activity has ended or that has vented from active star-forming regions into a porous interstellar medium.
25 pages, accepted to AJ
References in corpus (7)
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- Extra-Nuclear Starbursts: Young Luminous Hinge Clumps in Interacting Galaxies
- Revealing Efficient Dust-Formation at Low Metallicity in Extragalactic Carbon-Rich Wolf-Rayet Binaries
- Spatially resolved star formation image and the ULX population in NGC2207/IC2163
- Hot Diffuse Emission in the Nuclear Starburst Region of NGC 2903
- The nature of the symbiotic candidate 2MASS J07363415+6538548 in the field of NGC 2403
- Probing the Infrared/Radio correlation of the full IRAS Revised Bright Galaxy Sample with MeerKAT and the VLA