Published January 1990 | Version v1
Journal article

Nonthermal X-ray emission from 3C 273 - The core of a knotty problem?

  • 1. CNR, Istituto di Astrofisica Spaziale, Frascati (Italy)
  • 2. Southampton Univ. (England)

Description

The quasar 3C 273 was observed in the hard X-ray region of the spectrum (15-300 keV) during a stratospheric balloon flight on July 15, 1987. The emitted photon spectrum is well described by a single power law of photon index -1.61 which corresponds to a hard (20-200 keV) X-ray luminosity of 0.8 x 10 to the 47th ergs/s. This flux is consistent with the 1978/1979 HEAO 1 and AIT/MPI measurements and about a factor of three below the high state measured in 1981 (AIT/MPI). The implications of these results with respect to the location of the production site and mechanism are discussed. 26 refs

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
349
Series
Astrophys. J.
Journal Page Range
41-44
ISSN
0004-637X
CODEN
ASJOA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
21055588
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
EMISSION SPECTRA; HARD X RADIATION; QUASARS; RADIATION FLUX; SPECTROSCOPY; TELESCOPES; X-RAY SPECTRA
Descriptors DEC
COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; RADIATIONS; SPECTRA; X RADIATION