Observation of hard x-ray emission from GRO J1744-28 in the 20-200 keV band during declining phase

Advances in Space Research

Volumn 28, Issue 2-3, 2001, Pages 337-341

  Manchanda, R K ^a   Rao, A R ^a  

^a TATA INSTITUTE OF FUNDAMENTAL RESEARCH   (India)

Author keywords

[No Author keywords available]

Indexed keywords

BAND STRUCTURE; ELECTROMAGNETIC WAVE EMISSION; SPECTRUM ANALYSIS; TELESCOPES;

SPECTRAL INDEXES;

X RAY ANALYSIS;

SOLAR SYSTEM;

EID: 0035401881     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00430-6     Document Type: Article

References (12)

1. Hard X-ray bursts from GRO J1744-28. Observations by Konus-Wind and Konus-A experiments
2. Optical/Near-Infrared observations of GRO J1744-28
3. Evidence for 'Propellor' effecs in X-rays pulsars GX 1+4 and GRO J1744-28
4. A high sensitivity payload for balloon-borne hard X-ray astronomy
5. GRO J1744-28
6. Galactic center
7. A new type of transient high energy source in the direction of Galactic Centre
8. A comparison between the rapid burster and GRO J1744-28
9. A double peaked pulse profile observed in GX 1+4
10. Hard X-ray spectroscopy and pulsar phase analysis of bursting X-ray pulsar GRO J1744-28 with OSSE
11. On the nature of bursting X-ray pulsar GRO J1744-28
12. Quasi-Periodic X-ray brightness oscillations of GRO J1744-28