BlackCAT A Catalog of Stellar-Mass Black Holes in X-ray Binaries

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ID# 65

MAXI J1810-222

(Kennea2019a)

RA     (ICRS)     DEC

[hh:mm:ss.ss]          [dd:mm:ss.ss]

18:12:39.66  -22:19:25.0


ℓ                      b

[deg]                            [deg]

008.7695570  -01.98090632

Year of discovery: 2018  
(Negoro2018a)

# of outbursts after discovery: 1


Basic data

Distance [kpc] 6
0.73±0.03
Russell2022Kennea2019a
Distance to the plane (z) [kpc] Russell2022Kennea2019a
Orbital period (Porb) [h]
Peak X-ray flux [erg s-1 cm-2]
[keV]

[]
Outburst magnitude (AB)
Quiescent magnitude (AB)
E(B-V) [mag]
Spectral type


NOTES

MAXI J1810-222: The nature of the source is still unclear but Russell2022 support a BH primary based on the X-ray colour and soft-state spectral model.
Since its discovery in 2018, the system was reported to brighten and harden (see Russell2022 and Negoro2019e, Ducci2020).
Yang2023 reported a new X-ray outburst detected by LEIA in June 2023.




Optical/NIR magnitudes

Mag. Outburst (AB)
Mag. Quiescent (AB)
Aladin finding chart
Scroll to zoom. Set survey image in "Manage layers"
Default image: DSS2 Red
MAXI J1810-222 in Simbad


This research has made use of NASA's Astrophysics Data System (ADS), the SIMBAD database operated at CDS (Strasbourg, France) and APLpy
Please acknowledge the use of this catalogue in any published work you derive from it.

Last modified: 25 March 2024.