RA (ICRS) DEC
|
ℓ b
|
Distance [kpc] | >8.5 | Stiele2012 |
---|---|---|
Distance to the plane (z) [kpc] | >-0.2 | Stiele2012 |
Orbital period (Porb) [h] | ||
Peak X-ray flux [erg s-1 cm-2] [keV] |
1.43E-09 [2-10] |
Stiele2012 |
Outburst magnitude (AB) | z’∼20.7 | Rau2011a |
Quiescent magnitude (AB) | KsB2=21.8±0.2 | Lopez2019 |
E(B-V) [mag] | 3.518 | Kennea2011c |
Spectral type |
MAXI J1543-564: Rau2011a reported 3 possible objects (A, B and C) close or within the radio (Miller-Jones2011b) and X-ray (Kennea2011a) error circles. Lopez2019 resolved the star B into B1 and B2 which magnitudes are reported in the quiescence magnitude section. The ourburst magnitude reported by Rau2011a probably refers to B1+B2. |
|
|||
---|---|---|---|
z’∼20.7 | |||
Lopez2019 |
|||
HB1=20.5±0.2 | KsB1=20.7±0.2 | ||
HB2=21.7±0.2 | KsB2=21.8±0.2 |
Finding chart reference: Rau2011aLopez2019