The INTEGRAL view of the pulsating hard X-ray sky: from
accreting and transitional millisecond pulsars to
rotation-powered pulsars and magnetars

J 2020

The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars

PAPITTO, A., M. FALANGA, W. HERMSEN, S. MEREGHETTI, L. KUIPER et. al.

Basic information

Original name

The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars

Authors

PAPITTO, A., M. FALANGA, W. HERMSEN, S. MEREGHETTI, L. KUIPER, J. POUTANEN, E. BOZZO, F. AMBROSINO, F. COTI ZELATI, Vittorio DE FALCO (380 Italy, belonging to the institution), D. DE MARTINO, T. DI SALVO, P. ESPOSITO, C. FERRIGNO, M. FOROT, D. GÖTZ, C. GOUIFFES, R. IARIA, P. LAURENT, J. LI, Z. LI, T. MINEO, P. MORAN, A. NERONOV, A. PAIZIS, N. REA, A. RIGGIO, A. SANNA, V. SAVCHENKO, A. SŁOWIKOWSKA, A. SHEARER, A. TIENGO and D. F. TORRES

Edition

New Astronomy Reviews, 2020, 1387-6473

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Country of publisher

Netherlands

Confidentiality degree

není předmětem státního či obchodního tajemství

References:

URL

RIV identification code

RIV/47813059:19630/20:A0000094

Organization unit

Institute of physics in Opava

DOI

http://dx.doi.org/10.1016/j.newar.2020.101544

UT WoS

000598886100001

Keywords in English

Accretion disks; Magnetars; Neutron stars; Pulsars; X-rays: binaries; X-rays: bursts

Abstract

V originále

In the last 25 years a new generation of X-ray satellites imparted a significant leap forward in our knowledge of X-ray pulsars. The discovery of accreting and transitional millisecond pulsars proved that disk accretion can spin up a neutron star to a very high rotation speed. The detection of MeV-GeV pulsed emission from a few hundreds of rotation-powered pulsars probed particle acceleration in the outer magnetosphere, or even beyond. Also, a population of two dozens of magnetars has emerged. INTEGRAL played a central role to achieve these results by providing instruments with high temporal resolution up to the hard X-ray/soft, gamma-ray band and a large field of view imager with good angular resolution to spot hard X-ray transients. In this article we review the main contributions by INTEGRAL to our understanding of the pulsating hard X-ray sky, such as the discovery and characterization of several accreting and transitional millisecond pulsars, the generation of the first catalog of hard X-ray/soft gamma-ray rotation-powered pulsars, the detection of polarization in the hard X-ray emission from the Crab pulsar, and the discovery of persistent hard X-ray emission from several magnetars.

Citovat

PAPITTO, A., M. FALANGA, W. HERMSEN, S. MEREGHETTI, L. KUIPER, J. POUTANEN, E. BOZZO, F. AMBROSINO, F. COTI ZELATI, Vittorio DE FALCO, D. DE MARTINO, T. DI SALVO, P. ESPOSITO, C. FERRIGNO, M. FOROT, D. GÖTZ, C. GOUIFFES, R. IARIA, P. LAURENT, J. LI, Z. LI, T. MINEO, P. MORAN, A. NERONOV, A. PAIZIS, N. REA, A. RIGGIO, A. SANNA, V. SAVCHENKO, A. SŁOWIKOWSKA, A. SHEARER, A. TIENGO and D. F. TORRES. The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars. New Astronomy Reviews. 2020, vol. 91, December, p. "101544-1"-"101544-26", 26 pp. ISSN 1387-6473. Available from: https://dx.doi.org/10.1016/j.newar.2020.101544.

@article{49621,
   author = {Papitto, A. and Falanga, M. and Hermsen, W. and Mereghetti, S. and Kuiper, L. and Poutanen, J. and Bozzo, E. and Ambrosino, F. and Coti Zelati, F. and De Falco, Vittorio and de Martino, D. and Di Salvo, T. and Esposito, P. and Ferrigno, C. and Forot, M. and Götz, D. and Gouiffes, C. and Iaria, R. and Laurent, P. and Li, J. and Li, Z. and Mineo, T. and Moran, P. and Neronov, A. and Paizis, A. and Rea, N. and Riggio, A. and Sanna, A. and Savchenko, V. and Słowikowska, A. and Shearer, A. and Tiengo, A. and Torres, D. F.},
   article_number = {December},
   doi = {http://dx.doi.org/10.1016/j.newar.2020.101544},
   keywords = {Accretion disks; Magnetars; Neutron stars; Pulsars; X-rays: binaries; X-rays: bursts},
   language = {eng},
   issn = {1387-6473},
   journal = {New Astronomy Reviews},
   title = {The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars},
   url = {https://www.sciencedirect.com/science/article/pii/S138764732030021X},
   volume = {91},
   year = {2020}
}

TY  - JOUR
ID  - 49621
AU  - Papitto, A. - Falanga, M. - Hermsen, W. - Mereghetti, S. - Kuiper, L. - Poutanen, J. - Bozzo, E. - Ambrosino, F. - Coti Zelati, F. - De Falco, Vittorio - de Martino, D. - Di Salvo, T. - Esposito, P. - Ferrigno, C. - Forot, M. - Götz, D. - Gouiffes, C. - Iaria, R. - Laurent, P. - Li, J. - Li, Z. - Mineo, T. - Moran, P. - Neronov, A. - Paizis, A. - Rea, N. - Riggio, A. - Sanna, A. - Savchenko, V. - Słowikowska, A. - Shearer, A. - Tiengo, A. - Torres, D. F.
PY  - 2020
TI  - The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars
JF  - New Astronomy Reviews
VL  - 91
IS  - December
SP  - "101544-1"-"101544-26"
EP  - "101544-1"-"101544-26"
SN  - 13876473
KW  - Accretion disks
KW  - Magnetars
KW  - Neutron stars
KW  - Pulsars
KW  - X-rays: binaries
KW  - X-rays: bursts
UR  - https://www.sciencedirect.com/science/article/pii/S138764732030021X
N2  - In the last 25 years a new generation of X-ray satellites imparted a significant leap forward in our knowledge of X-ray pulsars. The discovery of accreting and transitional millisecond pulsars proved that disk accretion can spin up a neutron star to a very high rotation speed. The detection of MeV-GeV pulsed emission from a few hundreds of rotation-powered pulsars probed particle acceleration in the outer magnetosphere, or even beyond. Also, a population of two dozens of magnetars has emerged. INTEGRAL played a central role to achieve these results by providing instruments with high temporal resolution up to the hard X-ray/soft, gamma-ray band and a large field of view imager with good angular resolution to spot hard X-ray transients. In this article we review the main contributions by INTEGRAL to our understanding of the pulsating hard X-ray sky, such as the discovery and characterization of several accreting and transitional millisecond pulsars, the generation of the first catalog of hard X-ray/soft gamma-ray rotation-powered pulsars, the detection of polarization in the hard X-ray emission from the Crab pulsar, and the discovery of persistent hard X-ray emission from several magnetars.
ER  -

PAPITTO, A., M. FALANGA, W. HERMSEN, S. MEREGHETTI, L. KUIPER, J. POUTANEN, E. BOZZO, F. AMBROSINO, F. COTI ZELATI, Vittorio DE FALCO, D. DE MARTINO, T. DI SALVO, P. ESPOSITO, C. FERRIGNO, M. FOROT, D. GÖTZ, C. GOUIFFES, R. IARIA, P. LAURENT, J. LI, Z. LI, T. MINEO, P. MORAN, A. NERONOV, A. PAIZIS, N. REA, A. RIGGIO, A. SANNA, V. SAVCHENKO, A. SŁOWIKOWSKA, A. SHEARER, A. TIENGO and D. F. TORRES. The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars. \textit{New Astronomy Reviews}. 2020, vol.~91, December, p.~''101544-1''-''101544-26'', 26 pp. ISSN~1387-6473. Available from: https://dx.doi.org/10.1016/j.newar.2020.101544.

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