The accretion mode in sub-eddington supermassive black holes: getting into the 
central parsecs of Andromeda

Alig, C.; Prieto, A.; Blaña, M.; Frischman, M.; Metzl, C.; Burkert, A.; Zier, O.; Streblyanska, A.

doi:10.3847/1538-4357/ace2c3

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

The accretion mode in sub-eddington supermassive black holes: getting into the central parsecs of Andromeda

MPS-Authors

/persons/resource/persons4664

Alig, C.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons145993

Blaña, M.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4602

Burkert, A.
Optical and Interpretative Astronomy, 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

Alig, C., Prieto, A., Blaña, M., Frischman, M., Metzl, C., Burkert, A., et al. (2023). The accretion mode in sub-eddington supermassive black holes: getting into the central parsecs of Andromeda. The Astrophysical Journal, 953(1): 109. doi:10.3847/1538-4357/ace2c3.

Cite as: https://hdl.handle.net/21.11116/0000-000E-7BE7-4

Abstract

There is no abstract available