IAFE   05512
INSTITUTO DE ASTRONOMIA Y FISICA DEL ESPACIO
Unidad Ejecutora - UE
artículos
Título:
Study of the γ-ray source 1AGL J2022+4032 in the Cygnus region
Autor/es:
CHEN, A.; PIANO, G.; TAVANI, M.; TROIS, A.; DUBNER, G.; GIACANI, E. & 55 COAUTHORS
Revista:
ASTRONOMY AND ASTROPHYSICS
Editorial:
EDP SCIENCES S A
Referencias:
Año: 2011 vol. 525 p. 33 - 40
ISSN:
0004-6361
Resumen:
Context. Identification of γ-ray-emitting Galactic sources is a
long-standing problem in astrophysics. One such source, 1AGL J2022+4032,
coincident with the interior of the radio shell of the supernova remnant
Gamma Cygni (SNR G78.2+2.1) in the Cygnus region, has recently been
identified by Fermi as a γ-ray pulsar, LAT PSR J2021+4026.
Aims: We present long-term observations of 1AGL J2022+4032 with the
AGILE γ-ray telescope, measuring its flux and light curve.
Methods: We compare the light curve of 1AGL J2022+4032 with that of 1AGL
J2021+3652 (PSR J2021+3651), showing that the flux variability of 1AGL
J2022+4032 appears to be greater than the level predicted from
statistical and systematic effects and producing detailed simulations to
estimate the probability of the apparent observed variability.
Results: We evaluate the possibility that the γ-ray emission may
be due to the superposition of two or more point sources, some of which
may be variable, considering a number of possible counterparts.
Conclusions: We consider the possibility of a nearby X-ray quiet
microquasar contributing to the flux of 1AGL J2022+4032 to be more
likely than the hypotheses of a background blazar or intrinsic
γ-ray variabilty of LAT PSR J2021+4026.