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Suzaku observation of two ultraluminous x-ray sources in ngc 1313 (Document No: 20070017443)
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Mizuno, T. Miyamoto, M. Isobe, N. Winter, L. Miyawaki, R. Ebisawa, K. Kubota, A. Petre, R. Dewangan, G. Mushotzky, R. F. Ueda, Y. |
| Copyright Year | 2007 |
| Description | TA study was made of two ultraluminous X-ray sources (ULXs) in the nearby faceon, late-type Sb galaxy NGC 1313 using data from Suzaku, the 5th Japanese X-ray satellite. Within the 90 ks observation, both sources named X-1 and X-2 exhibited luminosity change by about 50%. The o.4-10keV X-ray luminosity was measured. For X-1, the spectrum exhibited a strong power-law component with a high energy cutoff which is thought to arise from strong Comptonization by a disk corona, suggesting the source was in a very high state. Absorption line features with equivalent widths of 40-80 eV found at 7.00 keV and 7.8 keV in the X-1 spectrum support the presence of a highly ionized plasma and a high mass accretion rate on the system. The spectrum of X-2 in fainter phase is presented by a multicolor disk blackbody model. |
| File Size | 5903365 |
| Page Count | 23 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20070017443 |
| Archival Resource Key | ark:/13960/t5fc01t05 |
| Language | English |
| Publisher Date | 2007-01-01 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Coronas Luminosity Line Spectra Compton Effect Accretion Disks Black Holes Astronomy X Ray Sources Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |