AGN in the XMM-Newton first-light image as probes for the interstellar medium in the LMC

F. Haberl, K. Dennerl, M. D. Filipovic, B. Aschenbach, W. Pietsch, J. Trümper

Research output: Contribution to journalLetterpeer-review

10 Citations (Scopus)

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 languageEnglish
Pages (from-to)L208-L211
JournalAstronomy and Astrophysics
Volume365
Issue number1
DOIs
Publication statusPublished - Jan 2001

Keywords

  • Galaxies: LMC
  • Quasars: general
  • X-rays: ISM

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