IXPE Observations of the Quintessential Wind-accreting X-Ray Pulsar Vela X-1
Abstrak
The radiation from accreting X-ray pulsars was expected to be highly polarized, with some estimates for the polarization degree of up to 80%. However, phase-resolved and energy-resolved polarimetry of X-ray pulsars is required in order to test different models and to shed light on the emission processes and the geometry of the emission region. Here we present the first results of the observations of the accreting X-ray pulsar Vela X-1 performed with the Imaging X-ray Polarimetry Explorer. Vela X-1 is considered to be the archetypal example of a wind-accreting, high-mass X-ray binary system, consisting of a highly magnetized neutron star accreting matter from its supergiant stellar companion. The spectropolarimetric analysis of the phase-averaged data for Vela X-1 reveals a polarization degree (PD) of 2.3% ± 0.4% at the polarization angle (PA) of −47.°3 ± 5.°4. A low PD is consistent with the results obtained for other X-ray pulsars and is likely related to the inverse temperature structure of the neutron star atmosphere. The energy-resolved analysis shows the PD above 5 keV reaching 6%–10% and a ∼90° difference in the PA compared to the data in the 2–3 keV range. The phase-resolved spectropolarimetric analysis finds a PD in the range 0%–9% with the PA varying between −80° and 40°.
Topik & Kata Kunci
Penulis (101)
Sofia V. Forsblom
Juri Poutanen
Sergey S. Tsygankov
Matteo Bachetti
Alessandro Di Marco
Victor Doroshenko
Jeremy Heyl
Fabio La Monaca
Christian Malacaria
Herman L. Marshall
Fabio Muleri
Alexander A. Mushtukov
Maura Pilia
Daniele Rogantini
Valery F. Suleimanov
Roberto Taverna
Fei Xie
Iván Agudo
Lucio A. Antonelli
Luca Baldini
Wayne H. Baumgartner
Ronaldo Bellazzini
Stefano Bianchi
Stephen D. Bongiorno
Raffaella Bonino
Alessandro Brez
Niccolò Bucciantini
Fiamma Capitanio
Simone Castellano
Elisabetta Cavazzuti
Chien-Ting Chen
Stefano Ciprini
Enrico Costa
Alessandra De Rosa
Ettore Del Monte
Laura Di Gesu
Niccolò Di Lalla
Immacolata Donnarumma
Michal Dovčiak
Steven R. Ehlert
Teruaki Enoto
Yuri Evangelista
Sergio Fabiani
Riccardo Ferrazzoli
Javier A. Garcia
Shuichi Gunji
Kiyoshi Hayashida
Wataru Iwakiri
Svetlana G. Jorstad
Philip Kaaret
Vladimir Karas
Takao Kitaguchi
Jeffery J. Kolodziejczak
Henric Krawczynski
Luca Latronico
Ioannis Liodakis
Simone Maldera
Alberto Manfreda
Frédéric Marin
Andrea Marinucci
Alan P. Marscher
Giorgio Matt
Ikuyuki Mitsuishi
Tsunefumi Mizuno
Michela Negro
Chi-Yung Ng
Stephen L. O’Dell
Nicola Omodei
Chiara Oppedisano
Alessandro Papitto
George G. Pavlov
Abel L. Peirson
Matteo Perri
Melissa Pesce-Rollins
Pierre-Olivier Petrucci
Andrea Possenti
Simonetta Puccetti
Brian D. Ramsey
John Rankin
Ajay Ratheesh
Oliver J. Roberts
Roger W. Romani
Carmelo Sgrò
Patrick Slane
Paolo Soffitta
Gloria Spandre
Rashid A. Sunyaev
Douglas A. Swartz
Toru Tamagawa
Fabrizio Tavecchio
Yuzuru Tawara
Allyn F. Tennant
Nicholas E. Thomas
Francesco Tombesi
Alessio Trois
Roberto Turolla
Jacco Vink
Martin C. Weisskopf
Kinwah Wu
Silvia Zane
IXPE Collaboration
Akses Cepat
- Tahun Terbit
- 2023
- Sumber Database
- DOAJ
- DOI
- 10.3847/2041-8213/acc391
- Akses
- Open Access ✓