Literature Search

Great Balls of FIRE IV. The contribution of massive star clusters to the astrophysical population of merging binary black holes

#1

Tristan Bruel
(
)
,
Astrid Lamberts
(
- OCA, Nice, Lab. Lagrange and
- ARTEMIS, Nice
)
,
Carl L. Rodriguez
(
- UNC, Chapel Hill
)
,
Robert Feldmann
(
- U. Zurich (main)
)
,
Michael Y. Grudic
(
- CCA, New York
)

et al.

(Mar 5, 2025)

e-Print:
- 2503.03810 [astro-ph.GA]

pdf

reference search0 citations

Particle acceleration and multi-messenger radiation from Ultra-Luminous X-ray Sources -- A new class of Galactic PeVatrons

#2

Enrico Peretti
(
- APC, Paris
)
,
Maria Petropoulou
(
- Athens Natl. Capodistrian U. and
- Athens U.
)
,
Georgios Vasilopoulos
(
- Athens Natl. Capodistrian U. and
- Athens U.
)
,
Stefano Gabici
(
- APC, Paris
)

(Nov 13, 2024)

e-Print:
- 2411.08762 [astro-ph.HE]

pdf

reference search0 citations

An Empirical Framework Characterizing the Metallicity and Star-formation History Dependence of X-Ray Binary Population Formation and Emission in Galaxies

#3

et al.

(Oct 25, 2024)

Published in:
- Astrophys.J. 977 (2024) 2, 189
•
e-Print:
- 2410.19901 [astro-ph.GA]

DOI

reference search2 citations

Ultraluminous X-ray sources with He star companions

#4

et al.

(Oct 17, 2024)

Published in:
- Mon.Not.Roy.Astron.Soc. 534 (2024) 4, 3400-3409
•
e-Print:
- 2411.00407 [astro-ph.SR]

DOI

reference search1 citation

Possible Supercritical Accretion on the Ultraluminous X-Ray Source in the Metal-poor Galaxy I Zw 18

#5

(May 21, 2024)

Published in:
- Astrophys.J. 970 (2024) 1, 8
•
e-Print:
- 2405.13107 [astro-ph.HE]

DOI

reference search1 citation

The boring history of Gaia BH3 from isolated binary evolution

#6

Giuliano Iorio
(
- Padua U., Astron. Dept. and
- INFN, Padua
)
,
Stefano Torniamenti
(
- INFN, Padua and
- ZAH, Heidelberg
)
,
Michela Mapelli
(
- Padua U., Astron. Dept. and
- INFN, Padua and
- ZAH, Heidelberg
)
,
Marco Dall'Amico
(
- Padua U., Astron. Dept. and
- INFN, Padua
)
,
Alessandro A. Trani
(
- Bohr Inst.
)

et al.

(Apr 26, 2024)

Published in:
- Astron.Astrophys. 690 (2024) A144,
- Astron.Astrophys. 690 (2024) A144
•
e-Print:
- 2404.17568 [astro-ph.GA]

DOI

reference search7 citations

The High-mass X-Ray Binary Luminosity Functions of Dwarf Galaxies

#7

(Jan 25, 2024)

Published in:
- Astrophys.J. 965 (2024) 1, 67
•
e-Print:
- 2401.14477 [astro-ph.GA]

DOI

reference search3 citations

Monitoring the X-Ray Variability of Bright X-Ray Sources in M33

#8

et al.

(Dec 5, 2023)

Published in:
- Astrophys.J. 961 (2024) 2, 168
•
e-Print:
- 2312.03075 [astro-ph.HE]

DOI

reference search0 citations

The high energy X-ray probe: resolved X-ray populations in extragalactic environments

#9

et al.

(Oct 30, 2023)

Published in:
- Front.Astron.Space Sci. 10 (2023) 1293918
•
e-Print:
- 2311.04735 [astro-ph.HE]

DOI

reference search3 citations

Evidence of evolution of the black hole mass function with redshift

#10

(Oct 4, 2023)

Published in:
- Astron.Astrophys. 684 (2024) A204
•
e-Print:
- 2310.03074 [astro-ph.HE]

DOI

reference search32 citations

Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations

#11

et al.

(Sep 27, 2023)

Published in:
- Astron.Astrophys. 682 (2024) A69,
- Astron.Astrophys. 682 (2024) A69
•
e-Print:
- 2309.15904 [astro-ph.HE]

DOI

reference search9 citations

The Black Hole Mass Function: From Stellar to Supermassive

#12

ALEXANDER MARC. Sicilia

(Sep 26, 2023)

reference search0 citations

Population synthesis of Be X-ray binaries: metallicity dependence of total X-ray outputs

#13

(Aug 11, 2023)

e-Print:
- 2308.06154 [astro-ph.HE]

pdf

reference search1 citation

Modeling the High-energy Ionizing Output from Simple Stellar and X-Ray Binary Populations

#14

et al.

(Jun 30, 2023)

Published in:
- Astrophys.J. 960 (2024) 1, 13
•
e-Print:
- 2307.00050 [astro-ph.GA]

DOI

reference search7 citations

The evolution of compact objects and thier host galaxies across cosmic time

#15

Filippo Santoliquido
(
- U. Padua (main)
)

(Apr 3, 2023)

links

reference search0 citations

The largest bright ULX population in a galaxy: X-ray variability and luminosity function in the Cartwheel ring galaxy

#16

(Mar 27, 2023)

Published in:
- Mon.Not.Roy.Astron.Soc. 522 (2023) 1, 1377-1393
•
e-Print:
- 2303.15502 [astro-ph.HE]

pdfDOI

reference search3 citations

Ultraluminous X-ray sources

#17

Andrew King
(
- Leicester U. and
- Amsterdam U., Astron. Inst. and
- Leiden Observ.
)
,
Jean-Pierre Lasota
(
- Paris, Inst. Astrophys. and
- Warsaw, Copernicus Astron. Ctr.
)
,
Matthew Middleton
(
- Southampton U.
)

(Jan 7, 2023)

Published in:
- New Astron.Rev. 96 (2023) 101672
•
e-Print:
- 2302.10605 [astro-ph.HE]

pdfDOI

reference search83 citations

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

#18

et al.

(Jan 3, 2023)

Published in:
- Mon.Not.Roy.Astron.Soc. 519 (2023) 4, 5848-5858
•
e-Print:
- 2301.01317 [astro-ph.HE]

pdfDOI

reference search5 citations

The first pieces of the gravitational-wave progenitor population puzzle

#19

A.A.C. van Son
(
- Amsterdam U.
)

(2023)

links

reference search0 citations

The ionizing and heating power of ultraluminous X-ray sources under the geometrical beaming model

#20

K. Kovlakas
(
- U. Geneva (main)
)
,
T. Fragos
(
- U. Geneva (main)
)
,
D. Schaerer
(
- U. Geneva (main) and
- IRAP, Toulouse
)
,
A. Mesinger
(
- Pisa, Scuola Normale Superiore
)

(Jul 19, 2022)

Published in:
- Astron.Astrophys. 665 (2022) A28,
- Astron.Astrophys. 665 (2022) A28
•
e-Print:
- 2207.09331 [astro-ph.HE]

DOI

reference search13 citations

Chemical Evolution of the Universe and its Consequences for Gravitational-Wave Astrophysics

#21

Martyna Chruślińska

(Jun 21, 2022)

Published in:
- Annalen Phys. 536 (2024) 2, 2200170
•
e-Print:
- 2206.10622 [astro-ph.GA]

DOI

reference search39 citations

BLACK HOLE OR NEUTRON STAR? THIS IS (ONE OF) THE QUESTION(S) A VARIABILITY STUDY OF ULXs TOWARDS A BETTER COMPREHENSION OF THEIR PHYSICS

#22

C. Salvaggio

(May 6, 2022)

pdf

reference search0 citations

The Redshift Evolution of Ultraluminous X-Ray Sources out to z ∼ 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background

#23

(May 2, 2022)

Published in:
- Astrophys.J. 932 (2022) 1, 27
•
e-Print:
- 2205.01127 [astro-ph.GA]

DOI

reference search2 citations

Modelling the formation of the first two neutron star–black hole mergers, GW200105 and GW200115: metallicity, chirp masses, and merger remnant spins

#24

(Mar 11, 2022)

Published in:
- Mon.Not.Roy.Astron.Soc. 513 (2022) 4, 5780-5789
•
e-Print:
- 2203.05850 [astro-ph.HE]

pdfDOI

reference search20 citations

The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields

#25

et al.

(Dec 6, 2021)

Published in:
- Astrophys.J. 926 (2022) 1, 28
•
e-Print:
- 2112.03194 [astro-ph.HE]

DOI

reference search11 citations

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