The X-ray lightcurve of Sagittarius A* over the past 150 years inferred from 
Fe-Kα line reverberation in galactic centre molecular clouds

Capelli, R.; Warwick, R. S.; Porquet, D.; Gillessen, S.; Predehl, P.

doi:10.1051/0004-6361/201219544

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

The X-ray lightcurve of Sagittarius A* over the past 150 years inferred from Fe-Kα line reverberation in galactic centre molecular clouds

MPS-Authors

/persons/resource/persons20173

Capelli, R.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4768

Gillessen, S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4831

Predehl, P.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Capelli, R., Warwick, R. S., Porquet, D., Gillessen, S., & Predehl, P. (2012). The X-ray lightcurve of Sagittarius A* over the past 150 years inferred from Fe-Kα line reverberation in galactic centre molecular clouds. Astronomy & Astrophysics, 545: A35, pp. 1-22. doi:10.1051/0004-6361/201219544.

Cite as: https://hdl.handle.net/11858/00-001M-0000-000E-7C42-D

Abstract

There is no abstract available