Radio observations of the region around the pulsar wind nebula HESS J1303−631 with ATCA - INSPIRE

DataBETA

Radio observations of the region around the pulsar wind nebula HESS J1303−631 with ATCA

Iurii Sushch
(
- Potchefstroom U. and
- DESY, Zeuthen and
- Lvov Nat. U.
)
,
Igor Oya
(
- DESY, Zeuthen
)
,
Ullrich Schwanke
(
- Humboldt U., Berlin
)
,
Simon Johnston
(
- Australia, CSIRO, Epping
)
,
Matthew L. Dalton
(
- Unlisted, DE
)

Jun 19, 2017

7 pages

Published in:

Astron.Astrophys. 605 (2017) A115

Published: Sep 1, 2017

e-Print:

1706.05891 [astro-ph.HE]

DOI:

10.1051/0004-6361/201527871

Experiments:

ATCA

View in:

ADS Abstract Service

reference search5 citations

Citations per year

Abstract: (EDP Sciences)

Radio observations of the region surrounding PSR J1301−6305 at 5.5 GHz and 7.5 GHz were conducted with ATCA on September 5, 2013. The observations were dedicated to the search of the radio counterpart of the evolved pulsar wind nebula (PWN) HESS J1303−631, which has been detected in X-rays and GeV–TeV γ-rays. The collected data do not reveal any significant extended emission associated with PSR J1301−6305. In addition, archival 1.384 GHz and 2.368 GHz data do not show any evidence for a radio counterpart of HESS J1303−631. Archival 1.384 GHz observations reveal the detection of an extended structure centred at an angular distance of 19′ from the pulsar. This extended structure might be a supernova remnant (SNR) and a potential birth place of PSR J1301−6305. The implications of the lack of a radio counterpart of HESS J1303−631 on the understanding of the nature of the PWN are discussed. Key words: radiation mechanisms: non-thermal / radio continuum: stars / pulsars: individual: PSR J1301 / 6305 / stars: winds, outflows

Note:

7 pages, 4 figures, 2 tables, accepted for publication in A&A

pulsars: individual: PSR J1301 − 6305
stars: winds, outflows
radiation mechanisms: non-therma
radiation mechanisms: non-thermal
radio continuum: stars
pulsars: individual: PSR J1301
6305
HESS
pulsar
structure

References(44)

Figures(6)

Constraints on the Galactic Population of TeV Pulsar Wind Nebulae Using $FERMI$ Large Area Telescope Observations

F. Acero
(
- NASA, Goddard
)
,
M. Ackermann
(
- DESY, Zeuthen
)
,
M. Ajello
(
- UC, Berkeley, Space Sci. Dept.
)
,
A. Allafort
(
- KIPAC, Menlo Park and
- SLAC
)
,
L. Baldini
(
- INFN, Pisa and
- Pisa U.
)

et al.

- Astrophys.J. 773 (2013) 77
•
e-Print:
- 1306.5735
•
DOI:
- 10.1088/0004-637X/773/1/77

Serendipitous discovery of the unidentified extended TeV gamma-ray source HESS J1303-631

H.E.S.S.

Collaboration

•

F. Aharonian

et al.

- Astron.Astrophys. 439 (2005) 1013-1021
•
e-Print:
- astro-ph/0505219
•
DOI:
- 10.1051/0004-6361:20053195

A High Braking Index for a Pulsar

et al.

- Astrophys.J.Lett. 819 (2016) 1, L16
•
e-Print:
- 1603.00305
•
DOI:
- 10.3847/2041-8205/819/1/L16

GLIMPSE: 1. A SIRTF legacy project to map the inner galaxy

et al.

- Publ.Astron.Soc.Pac. 115 (2003) 953-964
•
e-Print:
- astro-ph/0306274
•
DOI:
- 10.1086/376696

Pulsar wind nebulae in evolved supernova remnants

- Astrophys.J. 563 (2001) 806
•
e-Print:
- astro-ph/0107076
•
DOI:
- 10.1086/324042

Pulsar bow shock nebulae. 3. Inclusion of a neutral component, and H(alpha) luminosity

N. Bucciantini
(
- Florence U.
)

- Astron.Astrophys. 393 (2002) 629-636
•
e-Print:
- astro-ph/0207016
•
DOI:
- 10.1051/0004-6361:20020968

N. Bucciantini
,
R. Bandiera

- Astron.Astrophys. 375 (2001) 1032

J.J. Condon
,
M.R. Griffith
,
A.E. Wright

- Astron.J. 106 (1993) 1095

Neutron star population dynamics. 2. 3-D space velocities of young pulsars

- Astrophys.J. 505 (1998) 315-338
•
e-Print:
- astro-ph/9707308
•
DOI:
- 10.1086/306138

VizieR Online Data

R.M. Cutri
,
M.F. Skrutskie
,
S. van Dyk

Unidentified Gamma-Ray Sources as Ancient Pulsar Wind Nebulae

et al.

e-Print:
- 0906.2644

Radio emission from Supernova Remnants

Gloria Dubner
(
- Buenos Aires, IAFE
)
,
Elsa Giacani
(
- Buenos Aires, IAFE
)

- Astron.Astrophys.Rev. 23 (2015) 1, 3
•
e-Print:
- 1508.07294
•
DOI:
- 10.1007/s00159-015-0083-5

Particle Acceleration in Supernova Remnants and the Production of Thermal and Nonthermal Radiation

- Astrophys.J. 661 (2007) 879-891
•
e-Print:
- astro-ph/0702674
•
DOI:
- 10.1086/517518

The evolution and structure of pulsar wind nebulae

- Ann.Rev.Astron.Astrophys. 44 (2006) 17-47
•
e-Print:
- astro-ph/0601081
•
DOI:
- 10.1146/annurev.astro.44.051905.092528

Supernova Remnant Kes 17: Efficient Cosmic Ray Accelerator inside a Molecular Cloud

Joseph D. Gelfand
(
- New York U., CCPP
)
,
Daniel Castro
(
- MIT, MKI
)
,
Patrick O. Slane
(
- Harvard-Smithsonian Ctr. Astrophys.
)
,
Tea Temim
(
- NASA, Goddard and
- JIHIR, Oak Ridge
)
,
John P. Hughes
(
- Rutgers U., Piscataway
)

et al.

- Astrophys.J. 777 (2013) 2, 148
•
e-Print:
- 1311.6894
•
DOI:
- 10.1088/0004-637X/777/2/148

in Astronomical Society of the Pacific Conference Series, Vol. 77, Astronomical Data Analysis Software and Systems IV, ed. R. A

R. Gooch

Payne, & J. J. E. Hayes 144

H.E. Shaw

A.J. Green
,
S.N. Reeves
,
T. Murphy

- Publ.Astron.Soc.Austral. 31 (2014) e042

A catalogue of 294 Galactic supernova remnants

D.A. Green

- Bull.Astron.Soc.India 42 (2014) 47
•
e-Print:
- 1409.0637

M.R. Griffith
,
A.E. Wright

- Astron.J. 105 (1993) 1666

Identification of HESS J1303-631 as a Pulsar Wind Nebula through gamma-ray, X-ray and radio observations

H.E.S.S.

Collaboration

•

A. Abramowski

et al.

- Astron.Astrophys. 548 (2012) A46
•
e-Print:
- 1210.6513
•
DOI:
- 10.1051/0004-6361/201219814

Pulsar-Wind Nebulae: Recent Progress in Observations and Theory

- Space Sci.Rev. 191 (2015) 1-4, 391-439
•
e-Print:
- 1507.03662
•
DOI:
- 10.1007/s11214-015-0171-x

45 years of rotation of the Crab pulsar

et al.

- Mon.Not.Roy.Astron.Soc. 446 (2015) 857-864
•
e-Print:
- 1410.0886
•
DOI:
- 10.1093/mnras/stu2118

The Australia Telescope National Facility pulsar catalogue

R N Manchester
(
- Australia, CSIRO, Epping
)
,
G B Hobbs
(
- Australia, CSIRO, Epping
)
,
A Teoh
(
- Australia, CSIRO, Epping
)
,
M Hobbs
(
- Australia, CSIRO, Epping
)

- Astron.J. 129 (2005) 1993
•
e-Print:
- astro-ph/0412641
•
DOI:
- 10.1086/428488

Z. Misanovic
,
L. Cram
,
A. Green

- Mon.Not.Roy.Astron.Soc. 335 (2002) 114

1-25 of 44
1
2
25 / page