7 research outputs found
Investigating the region of 3C 397 in High Energy Gamma rays
We investigate the supernova remnant (SNR) 3C 397 and its neighboring pulsar
PSR J1906+0722 in high energy gamma rays by using nearly six years of archival
data of {\it Large Area Telescope} on board {\it Fermi Gamma Ray Space
Telescope} (Fermi-LAT). The off-pulse analysis of gamma-ray flux from the
location of PSR J1906+0722 reveals an excess emission which is found to be very
close to the radio location of 3C 397. Here, we present the preliminary results
of this gamma-ray analysis of 3C 397 and PSR J1906+0722.Comment: 4 pages, 3 figures, Proceeding of IAU Symposium No. 331, 201
A New Gamma-Ray Source in the Vicinity of the Galactic Supernova Remnant G306.30.9
A new extended gamma-ray source, which was named as Source A, in the
southwest of Galactic supernova remnant (SNR) G306.30.9 was detected with a
significance of 13 at the location of R.A. (J2000) =
13 17 52.80, Decl. (J2000) =
63 55 48.00 using about 9 years of Fermi-LAT data. In
order to investigate this unidentified gamma-ray source in multi-wavelengths,
we performed Swift observations of Source A. In this presentation we summarize
the published gamma-ray results, report about the recent ToO Swift observations
of Source A, and show our preliminary results of the gamma-ray analysis that we
conducted using the new X-ray data.Comment: Published in proceedings of "7th Fermi Symposium 2017",
PoS(IFS2017)10
Discovery of recombining plasma inside the extended gamma-ray supernova remnant HB9
We present the results from the Suzaku X-ray Imaging Spectrometer observation
of the mixed-morphology supernova remnant (SNR) HB9 (G160.9+2.6). We discovered
recombining plasma (RP) in the western Suzaku observation region and the
spectra here are well described by a model having collisional ionization
equilibrium (CIE) and RP components. On the other hand, the X-ray spectra from
the eastern Suzaku observation region are best reproduced by the CIE and
non-equilibrium ionization model. We discuss possible scenarios to explain the
origin of the RP emission based on the observational properties and concluded
that the rarefaction scenario is a possible explanation for the existence of
RP. In addition, the gamma-ray emission morphology and spectrum within the
energy range of 0.2300 GeV are investigated using 10 years of data
from the Fermi Large Area Telescope (LAT). The gamma-ray morphology of HB9 is
best described by the spatial template of radio continuum emission. The
spectrum is well-fit to a log-parabola function and its detection significance
was found to be 25. Moreover, a new gamma-ray point source
located just outside the south-east region of the SNR's shell was detected with
a significance of 6. We also investigated the archival HI and CO
data and detected an expanding shell structure in the velocity range of
and km s that is coinciding with a region of gamma-ray
enhancement at the southern rim of the HB9 shell.Comment: 12 pages, 7 figures, accepted for publication in MNRA
A new gamma-ray source in the vicinity of the galactic supernova remnant G306.3-0.9
A new extended gamma-ray source, which was named as Source A, in the southwest of Galactic supernova remnant (SNR) G306.3-0.9 was detected with a significance of ~13ϭ at the location of R.A. (J2000) = 13h 17m 52s.80, Decl. (J2000) = -63° 55’ 48”.00 using about 9 years of Fermi-LAT data. In order to investigate this unidentified gamma-ray source in multi-wavelengths, we performed Swift observations of Source A. In this presentation we summarize the published gamma-ray results, report about the recent ToO Swift observations of Source A, and show our preliminary results of the gamma-ray analysis that we conducted using the new X-ray data