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Conference Paper: Searching for X-ray counterparts of fermi gamma-ray pulsars in suzaku observations
Title | Searching for X-ray counterparts of fermi gamma-ray pulsars in suzaku observations |
---|---|
Authors | |
Keywords | Gamma-Ray Pulsars. Fermi. Pulsar Pulsar Wind Nebulae |
Issue Date | 2011 |
Publisher | Cambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU |
Citation | Proceedings Of The International Astronomical Union, 2011, v. 7 S279, p. 317-318 How to Cite? |
Abstract | We report the Suzaku follow-up observations of the Gamma-ray pulsars, 1FGL J0614,13328, J1044.55737, J1741.82101, and J1813.31246, which were discovered by the Fermi Gamma-ray observatory. Analysing Suzaku/XIS data, we detected X-ray counterparts of these pulsars in the Fermi error circle and interpreted their spectra with absorbed power-law functions. These results indicate that the origin of these X-ray sources is non-thermal emission from the pulsars or from Pulsar Wind Nebulae (PWNe) surrounding them. Moreover we found that J1741.82101 exhibits a peculiar profile: spin-down luminosity vs flux ratio between X-and gamma-rays is unusually large compared to usual radio pulsars. © 2012 International Astronomical Union. |
Persistent Identifier | http://hdl.handle.net/10722/188514 |
ISSN | 2023 SCImago Journal Rankings: 0.121 |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
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dc.contributor.author | Aoki, Y | en_US |
dc.contributor.author | Enomoto, T | en_US |
dc.contributor.author | Yatsu, Y | en_US |
dc.contributor.author | Kawai, N | en_US |
dc.contributor.author | Nakamori, T | en_US |
dc.contributor.author | Kataoka, J | en_US |
dc.contributor.author | Saz Parkinson, P | en_US |
dc.date.accessioned | 2013-09-03T04:09:18Z | - |
dc.date.available | 2013-09-03T04:09:18Z | - |
dc.date.issued | 2011 | en_US |
dc.identifier.citation | Proceedings Of The International Astronomical Union, 2011, v. 7 S279, p. 317-318 | en_US |
dc.identifier.issn | 1743-9213 | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/188514 | - |
dc.description.abstract | We report the Suzaku follow-up observations of the Gamma-ray pulsars, 1FGL J0614,13328, J1044.55737, J1741.82101, and J1813.31246, which were discovered by the Fermi Gamma-ray observatory. Analysing Suzaku/XIS data, we detected X-ray counterparts of these pulsars in the Fermi error circle and interpreted their spectra with absorbed power-law functions. These results indicate that the origin of these X-ray sources is non-thermal emission from the pulsars or from Pulsar Wind Nebulae (PWNe) surrounding them. Moreover we found that J1741.82101 exhibits a peculiar profile: spin-down luminosity vs flux ratio between X-and gamma-rays is unusually large compared to usual radio pulsars. © 2012 International Astronomical Union. | en_US |
dc.language | eng | en_US |
dc.publisher | Cambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU | en_US |
dc.relation.ispartof | Proceedings of the International Astronomical Union | en_US |
dc.subject | Gamma-Ray Pulsars. Fermi. | en_US |
dc.subject | Pulsar | en_US |
dc.subject | Pulsar Wind Nebulae | en_US |
dc.title | Searching for X-ray counterparts of fermi gamma-ray pulsars in suzaku observations | en_US |
dc.type | Conference_Paper | en_US |
dc.identifier.email | Saz Parkinson, P: pablosp@hku.hk | en_US |
dc.identifier.authority | Saz Parkinson, P=rp01803 | en_US |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.doi | 10.1017/S1743921312013130 | en_US |
dc.identifier.scopus | eid_2-s2.0-84866261868 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-84866261868&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 7 | en_US |
dc.identifier.issue | S279 | en_US |
dc.identifier.spage | 317 | en_US |
dc.identifier.epage | 318 | en_US |
dc.identifier.isi | WOS:000393362200053 | - |
dc.publisher.place | United Kingdom | en_US |
dc.identifier.scopusauthorid | Aoki, Y=55358273700 | en_US |
dc.identifier.scopusauthorid | Enomoto, T=36052706400 | en_US |
dc.identifier.scopusauthorid | Yatsu, Y=10238844100 | en_US |
dc.identifier.scopusauthorid | Kawai, N=55191405000 | en_US |
dc.identifier.scopusauthorid | Nakamori, T=8273010400 | en_US |
dc.identifier.scopusauthorid | Kataoka, J=25637485000 | en_US |
dc.identifier.scopusauthorid | Saz Parkinson, P=8948464400 | en_US |
dc.identifier.issnl | 1743-9213 | - |