RA (ICRS) DEC
|
ℓ b
|
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 |
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. |
|
|||
---|---|---|---|
|
|||