Multiwavelength scrutiny of X-ray sources in dwarf galaxies: ULXs versus AGNs

Multiwavelength scrutiny of X-ray sources in dwarf galaxies: ULXs versus AGNs

Owing to their quiet evolutionary histories, nearby dwarf galaxies (stellar masses M∗ ≲ 3 × 109 M⊙) have the potential to teach us about the mechanism(s) that 'seeded' the growth of supermassive black holes, and also how the first stellar mass black holes formed and interacted with their e...

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Bibliographic Details
Main Authors: Thygesen, E., Plotkin, R.M., Soria, R., Reines, A.E., Greene, J.E., Anderson, Gemma, Baldassare, V.F., Owens, M.G., Urquhart, R.T., Gallo, E., Miller-Jones, James, Paul, J.D., Rollings, A.P.
Format: Journal Article
Language:English
Published: OXFORD UNIV PRESS 2023
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
stars: black holes
galaxies: dwarf
radio continuum: galaxies
X-rays: galaxies
STAR-FORMATION RATE
QUASAR LUMINOSITY FUNCTION
ACTIVE GALACTIC NUCLEI
DIGITAL-SKY-SURVEY
LOW-MASS GALAXIES
BLACK-HOLE
STELLAR MASS
FUNDAMENTAL PLANE
SEYFERT-1 GALAXY
FORMING GALAXIES
Online Access:http://purl.org/au-research/grants/arc/DE180100346
http://hdl.handle.net/20.500.11937/96439

Internet

http://purl.org/au-research/grants/arc/DE180100346
http://hdl.handle.net/20.500.11937/96439

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