Abstract
The XMM-Newton first-light image revealed X-ray point sources which show heavily absorbed power-law spectra. The spectral indices and the probable identification of a radio counterpart for the brightest source suggest AGN shining through the interstellar gas of the Large Magellanic Cloud (LMC). The column densities derived from the X-ray spectra in combination with H I measurements will allow to draw conclusions on H I to H2 ratios in the LMC and compare these with values found for the galactic plane.
| Original language | English |
|---|---|
| Pages (from-to) | L208-L211 |
| Journal | Astronomy and Astrophysics |
| Volume | 365 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - Jan 2001 |
Keywords
- Galaxies: LMC
- Quasars: general
- X-rays: ISM