Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-25T11:26:42.639Z Has data issue: false hasContentIssue false
  • English
  • Français

ROSAT Observations of Active Galactic Nuclei

Published online by Cambridge University Press:  19 July 2016

W. Brinkmann
W. Brinkmann*
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, D-85740 Garching, F. R. G.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The large number of Active Galactive Nuclei detected for the first time through their X-ray emission in the ROSAT All Sky Survey as well as the first measurements of the X-ray emission of many previously known AGN provide a new unprecedented large basis for the statistical and morphological exploration of these objects.

The soft energy range of the X-Ray Telescope, the good energy resolution of the PSPC detector, and the high sensitivity of the instrument further allows an investigation of the spectral properties of sources in this energetically important energy band.

A short overview is given of the actual ongoing research concentrating on the study of the soft X-ray class properties of the various types of AGN.

Keywords

Active Galactic NucleiX-raysUnification Schemes
Type
New Observations of AGN with Specific Instruments
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 53 - 62
Copyright
Copyright © Kluwer 1994 

References

1. Voges, W. 1992. in Proc. of the ISY Conference “Space Science” , ESA ISY-3, ESA Publications, p.9 Google Scholar
2. Pfeffermann, E., Briel, U.G., Hippmann, H., Kettenring, G., Metzner, G., Predehl, P., Reger, G., Stephan, K.H., Zombeck, M.V., Chappell, J., Murray, S.S., 1986, Proc SPIE 733, 519 CrossRefGoogle Scholar
3. Veron-Cetty, M.-P. and Veron, P., 1991, ESO Scientific Report No. 10.Google Scholar
4. Bade, N., Engels, D., Fink, H., Hagen, H.-J., Reimers, D., Voges, W., and Wisotzki, L., 1992, Astr. Astrophys. , 254, L21 Google Scholar
5. Large, M.I., Cram, L.E., & Burgess, A.M., 1991, The Observatory 111, 72.Google Scholar
6. Condon, J.J., Broderick, J.J., and Seielstad, G.A., 1989, Astron. J. 97, 1064.CrossRefGoogle Scholar
7. Brinkmann, W., 1992. in: Proc. of a Conference on “X-Ray Emission from AGN and the Cosmic X-Ray Background” , eds. Brinkmann, W. and Trümper, J., MPE Report 143.Google Scholar
8. Brinkmann, W., Siebert, J., and Boller, Th., 1993, Astr. Astrophys. , in press.Google Scholar
9. Brinkmann, W., and Siebert, J., 1993, Astr. Astrophys. , submitted.Google Scholar
10. Henry, J.P. et al., 1993, Astron. J. , submitted Google Scholar
11. Becker, R.H., Helfand, D.J., and White, R.L., 1992, Astron. J. , 104, 531.CrossRefGoogle Scholar
12. Antonucci, R., 1993, Ann. Rev. Astron. Astr. 31, 473.CrossRefGoogle Scholar
13. Pietsch, W., et al., 1993, Astr. Astrophys. , submitted Google Scholar
14. Kellermann, K.I., et al., 1989, Astron. J. , 98, 1195.CrossRefGoogle Scholar
15. Elvis, M., Schreier, E.J., Tonry, J., Davis, M., and Huchra, J.P., 1981, Astrophys. J. , 246, 20.CrossRefGoogle Scholar
16. Fabbiano, G., et al., 1984. Astrophys. J. 277, 115.CrossRefGoogle Scholar
17. Barthel, P.D., 1989. Astrophys. J. 336, 319.Google Scholar
18. Scheuer, P.A.G., 1987. in Superluminal Radio Sources , eds. Zensus, J.A. and Pearson, T.J., Cambridge Univ. Press, Cambridge, p. 104.Google Scholar
19. Pierre, M., Hunstead, R., and Unnewisse, A., 1993, in: Proc. of the NATO ASI ‘Clusters of Galaxies’, Münster, eds. Seitter, et al.Google Scholar