GRO J1750-27

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Other Name: AX J1749.1-2639 SIMBAD

Monitoring data: RXTE/ASM (only available)


Coordinates

RA 17h 49' 12.00", DEC -26° 38' 50.0"
RA 276.3000deg, DEC -26.6194deg
l 2.3682, b +0.5080

Binary system

Distance: 18 kpc ([1])

Orbit

Parameter Value Unit Reference
Porb 29.817(9) days [1]
tau 49931.02(1) MJD [1]
a sin i 101.8(5) lt-s [1]
e 0.360(2) [1]
omega 206.3(3) deg [1]

Description

Gro1750 mosaic.png

The Be transient GRO J1750-27 was discovered in 1995 during a major outburst [1]. The spin period of the neutron star of about 4.45 s was found to spin up during the outburst with a rate of 38 pHz/s, which is correlated to the luminosity.

The source appears to lie on the other side of the Galactic Centre and is very close on the celestial sphere to GX 3+1.

Spectrum

INTEGRAL observed the source during the second reported outburst in 2008. The spectrum could be modelled successfully with either a single cutoff powerlaw or thermal Comptonization. Additionally, the hardness decreased with time ([2]).

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 1.6 Scott, D. M., Finger, M. H., Wilson, R. B., 1997, ApJ, 488, 831 (NASA ADS)
  2. Shaw, S. E., Hill, A. B., Kuulkers, E., 2009, MNRAS, 393, 419 (NASA ADS)