2022MNRAS.516.2074F


Query : 2022MNRAS.516.2074F

2022MNRAS.516.2074F - Mon. Not. R. Astron. Soc., 516, 2074-2079 (2022/October-3)

The spin of new black hole candidate: MAXI J1803-298 observed by NuSTAR and NICER.

FENG Y., ZHAO X., LI Y., GOU L., JIA N., LIAO Z. and WANG Y.

Abstract (from CDS):

MAXI J1803-298, a newly-discovered Galactic transient, and black hole candidate was first detected by MAXI/GSC on 2021 May 01. In this paper, we present a detailed spectral analysis of MAXI J1803-298. Utilizing the X-ray reflection fitting method, we perform a joint fit to the spectra of MAXI J1803-298, respectively, observed by NuSTAR and NICER/XTI on the same day over the energy range between 0.7-79.0 keV in SIMS state, and the observed inner radius of the accretion disc is demonstrated to have extended to the ISCO radius (Rin =1.08 RISCO). Implementing the relativistic reflection model relxillCp, we found its spin (and the inclination angle i) can be constrained to be close to an extreme value, 0.991 (i ∼ 70 °), at 68 per cent confidence interval. The results suggest that MAXI J1803-298 may be a fast-rotating black hole with a large inclination angle.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): black hole physics - stars: individual: MAXI J1803-298 - X-rays: binaries

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 MAXI J1803-298 BH? 18 03 41.0 -29 48 14           ~ 69 0

Query : 2022MNRAS.516.2074F

Basic data :
MAXI J1803-298 -- Black Hole Candidate
Other object types:
otypes_help
BH? (2022ApJ), X (MAXI)
ICRS coord. (ep=J2000) :
18 03 41.0 -29 48 14 [ ] D 2021ATel14587....1S
FK4 coord. (ep=B1950 eq=1950) :
18 00 28.9 -29 48 23 [ ]
Gal coord. (ep=J2000) :
001.2381 -03.8350 [ ]
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Identifiers (1) :
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MAXI J1803-298

References (69 between 1850 and 2026) (Total 69)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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