New XMM-Newton analysis of three bright X-ray sources in M31 globular clusters, 
including a new black hole candidate

Barnard, R.; Stiele, H.; Hatzidimitriou, D.; Kong, A. K. H.; Williams, B. F.; Pietsch, W.; Kolb, U. C.; Haberl, F.; Sala, G.

doi:10.1086/592594

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

New XMM-Newton analysis of three bright X-ray sources in M31 globular clusters, including a new black hole candidate

MPS-Authors

/persons/resource/persons18648

Stiele, H.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons18594

Pietsch, W.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons16282

Haberl, F.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons20262

Sala, G.
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

Barnard, R., Stiele, H., Hatzidimitriou, D., Kong, A. K. H., Williams, B. F., Pietsch, W., et al. (2008). New XMM-Newton analysis of three bright X-ray sources in M31 globular clusters, including a new black hole candidate. The Astrophysical Journal, 689(2), 1215-1221. doi:10.1086/592594.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-C451-B

Abstract

There is no abstract available