Semantic Scholar Open Access 2025

A multiwavelength study of the Galactic center black hole candidate MAXI J1744-294

S. Mandel K. Mori P. Draghis Mark T. Reynolds C. Jin +70 lainnya

Abstrak

For the first time in nearly a decade, a bright transient was detected in the central parsec (pc) of the Galaxy. MAXI J1744-294, or -- as it was known in its previous life -- Swift J174540.2-290037, was discovered in outburst by the MAXI telescope in January 2025. We present the results of a broadband, multi-wavelength study of MAXI J1744-294, including data from the NuSTAR, Chandra, XMM-Newton, Swift, and NICER X-ray telescopes, as well as complementary radio and near-infrared observations. We analyze the changing X-ray emission as the outburst evolved from the high/soft to the low/hard state. Using relativistic reflection features in the data, we estimate a spin of $a>0.92$ and viewing inclination $\theta=28^{+3}_{-4}$ deg, consistent with the parameters measured for Swift J174540.2-290037. Based on the spectral and temporal characteristics of MAXI J1744-294, we reaffirm its classification as a candidate black hole (BH) low-mass X-ray binary (LMXB) -- the third candidate BH transient discovered within 20 arcsec of the Galactic supermassive black hole Sgr~A*. This work provides further evidence for a cusp of BH-LMXBs in the central pc of our Galaxy, as argued for in previous observational studies and suggested by analytical and theoretical work. Our ongoing multi-wavelength study, involving a complementary range of observatories and spanning different outburst states, can serve as a model for future time domain astrophysics research.

Topik & Kata Kunci

Penulis (75)

S

S. Mandel

K

K. Mori

P

P. Draghis

M

Mark T. Reynolds

C

C. Jin

M

M. Parra

B

B. Levin

E

Eric Miao

N

N. Grollimund

A

A. Ciurlo

S

Sean Granados

G

G. K. Jaisawal

L

L. Marra

M

M. Bachetti

F

F. Capitanio

N

N. Degenaar

C

C. Hailey

J

Jaesub Hong

S

S. Motta

G

G. Ponti

M

M. Shara

M

M. Shidatsu

J

J. Tomsick

R

Randall D. Campbell

S

S. Corbel

R

R. Fender

A

A. Ghez

J

J. Grindlay

D

Daryl Haggard

M

M. Hosek

Z

Ziqian Hua

O

Ole Konig

K

Kai Matsunaga

R

R. Mikuvsincov'a

M

M. Nynka

G

G. Sanger-Johnson

G

G. Stel

A

A. Tarana

R

R. Wijnands

S

Shuo Zhang Columbia Astrophysics Laboratory

M

M. I. F. Astrophysics

S

Space Research

D

D. O. Astronomy

O

O. University

N

National Astronomical Observatories

C

Chinese Academy of Sciences

D

D. Physics

E

E. University

U

Universit'e de Paris Cit'e

U

Universit'e Paris-Saclay

U

Ucla Department of Physics

A

Astronomy

D

Dtu Space

T

T. Denmark

I

I. D. A. E. P. Spaziali

I

I. D. Cagliari

A

A. S. M. F. Astronomy

U

U. Amsterdam

C

Center for Astrophysics Harvard Smithsonian

I

Inaf Brera

D

D. O. Astrophysics

A

A. History

S

Space Sciences Laboratory

U

U. California

B

Berkeley

W

W. Observatory

A

Astrophysics

U

U. Oxford

M

M. University

S

School of Physics Astronomy

S

S. Science

N

N. University

G

Graduate School of Science

K

Kyoto University

M

M. University

Format Sitasi

Mandel, S., Mori, K., Draghis, P., Reynolds, M.T., Jin, C., Parra, M. et al. (2025). A multiwavelength study of the Galactic center black hole candidate MAXI J1744-294. https://www.semanticscholar.org/paper/8b3fd6b30b51d9ee2788fc4e747a87296790203c

Akses Cepat

PDF tidak tersedia langsung

Cek di sumber asli →
Lihat di Sumber
Informasi Jurnal
Tahun Terbit
2025
Bahasa
en
Sumber Database
Semantic Scholar
Akses
Open Access ✓