The X-ray-faint early-type galaxy NGC 4697
| dc.contributor.author | Irwin, JA | |
| dc.contributor.author | Sarazin, CL | |
| dc.contributor.author | Bregman, JN | |
| dc.contributor.other | University of Michigan System | |
| dc.contributor.other | University of Michigan | |
| dc.contributor.other | University of Virginia | |
| dc.contributor.other | University of Alabama Tuscaloosa | |
| dc.date.accessioned | 2018-09-14T21:45:09Z | |
| dc.date.available | 2018-09-14T21:45:09Z | |
| dc.date.issued | 2000-11-20 | |
| dc.description.abstract | We analyze archival ROSAT HRI, ROSAT PSPC, and ASCA data of the X-ray-faint early-type galaxy NGC 4697. The joint ROSAT PSPC + ASCA spectrum is fitted by a two-component thermal model, a MEKAL model with kT(MEKAL) = 0.26(-0.03)(+0.04) keV with low metallicity and a bremsstrahlung model with kT(BREM) = 5.2(-1.6)(+3.0) keV. A similar model was found to fit the spectra of another faint early-type galaxy (NGC 4382) and the bulge of M31. We interpret this soft emission as a combination of emission from a soft component of low-mass X-ray binaries (LMXBs) and from a low-temperature interstellar medium, although the relative contributions of the two components could not be determined. Twelve point sources were identified within 4 ' of NGC 4697, of which 11 are most likely LMXBs associated with the galaxy. The soft X-ray colors of four of the LMXBs in NGC 4697 support the claim that LMXBs possess a soft spectral component. Finally, we present a simulation of what we believe the Chandra data of NGC 4697 will look like. | en_US |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | Irwin, J., Sarazin, C., Bregman, J. (2000): The X-Ray-Faint Early-Type Galaxy NGC 4697. The Astrophysical Journal Letters, 544(2). DOI: 10.1086/317196 | |
| dc.identifier.doi | 10.1086/317196 | |
| dc.identifier.uri | http://ir.ua.edu/handle/123456789/3874 | |
| dc.language | English | |
| dc.language.iso | en_US | |
| dc.publisher | IOP Publishing | |
| dc.subject | binaries : close | |
| dc.subject | galaxies : elliptical and lenticular, cD | |
| dc.subject | galaxies : ISM | |
| dc.subject | X-rays : galaxies | |
| dc.subject | X-rays : ISM | |
| dc.subject | X-rays : stars | |
| dc.subject | GAS IMAGING SPECTROMETER | |
| dc.subject | CCD SURFACE PHOTOMETRY | |
| dc.subject | ELLIPTIC GALAXIES | |
| dc.subject | EMISSION MECHANISMS | |
| dc.subject | COMPLETE SAMPLE | |
| dc.subject | ROSAT | |
| dc.subject | ASCA | |
| dc.subject | BINARIES | |
| dc.subject | SPECTRA | |
| dc.subject | M31 | |
| dc.subject | Astronomy & Astrophysics | |
| dc.title | The X-ray-faint early-type galaxy NGC 4697 | en_US |
| dc.type | text | |
| dc.type | Article |
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