Probing the polarized emission from SMC X-1: The brightest X-ray pulsar observed by IXPE Article Swipe
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· 2024
· Open Access
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· DOI: https://doi.org/10.1051/0004-6361/202450937
Recent observations of X-ray pulsars (XRPs) performed by the Imaging X-ray Polarimetry Explorer (IXPE) have made it possible to investigate the intricate details of these objects in a new way, thanks to the added value of X-ray polarimetry. Here we present the results of the IXPE observations of SMC X-1, a member of the small group of XRPs displaying super-orbital variability. SMC X-1 was observed by IXPE three separate times during the high state of its super-orbital period. The observed luminosity in the 2–8 keV energy band of L ∼ 2 × 10 38 erg s −1 makes SMC X-1 the brightest XRP ever observed by IXPE. We detect significant polarization in all three observations, with values of the phase-averaged polarization degree (PD) and polarization angle (PA) of 3.2 ± 0.8% and 97° ±8° for Observation 1, 3.0 ± 0.9% and 90° ±8° for Observation 2, and 5.5 ± 1.1% and 80° ±6° for Observation 3, for the spectro-polarimetric analysis. The observed PD shows an increase over time with decreasing luminosity, while the PA decreases in decrements of ∼10°. The phase-resolved spectro-polarimetric analysis reveals significant detection of polarization in three out of seven phase bins, with the PD ranging between ∼2% and ∼10%, and a corresponding range in the PA from ∼70° to ∼100°. The pulse-phase resolved PD displays an apparent anti-correlation with the flux. Using the rotating vector model, we obtain constraints on the pulsar’s geometrical properties for the individual observations. The position angle of the pulsar displays an evolution over time supporting the idea that we observe changes related to different super-orbital phases. Scattering in the wind of the precessing accretion disk may be responsible for the behavior of the polarimetric properties observed during the high-state of SMC X-1’s super-orbital period.
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- article
- Language
- en
- Landing Page
- https://doi.org/10.1051/0004-6361/202450937
- OA Status
- hybrid
- Cited By
- 12
- References
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- Related Works
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- OpenAlex ID
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https://openalex.org/W4402449540Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1051/0004-6361/202450937Digital Object Identifier
- Title
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Probing the polarized emission from SMC X-1: The brightest X-ray pulsar observed by IXPEWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2024Year of publication
- Publication date
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2024-09-11Full publication date if available
- Authors
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Sofia V. Forsblom, Sergey S. Tsygankov, Juri Poutanen, Victor Doroshenko, A. Alexander Mushtukov, Mason Ng, Swati Ravi, L. Marshall, Alessandro Di Marco, Fabio La Monaca, Christian Malacaria, Guglielmo Mastroserio, Vladislav Loktev, Andrea Possenti, F. Valery Suleimanov, Roberto Taverna, I. Agudo, A. Lucio Antonelli, Matteo Bachetti, L. Baldini, Helmut Baumgartner, R. Bellazzini, S. Bianchi, David Bongiorno, R. Bonino, A. Brez, N. Bucciantini, Fiamma Capitanio, Simone Castellano, E. Cavazzuti, Chien‐Ting Chen, S. Ciprini, E. Costa, Alessandra De Rosa, E. Del Monte, Laura Di Gesu, Niccolò Di Lalla, I. Donnarumma, Michal Dovčiak, Rainer Ehlert, Teruaki Enoto, Y. Evangelista, Sergio Fabiani, Riccardo Ferrazzoli, Adriana Garcia, Shuichi Gunji, Kiyoshi Hayashida, Jeremy Heyl, W. Iwakiri, Svetlana G. Jorstad, P. Kaaret, V. Karas, Fabian Kislat, Takao Kitaguchi, Jeffery J. Kolodziejczak, H. Krawczynski, L. Latronico, Ioannis Liodakis, S. Maldera, Alberto Manfreda, Frédéric Marin, Andrea Marinucci, Alan P. Marscher, F. Massaro, G. Matt, Ikuyuki Mitsuishi, Tsunefumi Mizuno, Fabio Muleri, Michela Negro, C.‐Y. Ng, Stephen L. O’Dell, N. Omodei, C. Oppedisano, Alessandro Papitto, George G. Pavlov, Abel L. Peirson, M. Perri, M. Pesce-Rollins, Pierre-Olivier Petrucci, M. Pilia, Simonetta Puccetti, Brian D. Ramsey, John Rankin, Ajay Ratheesh, O. J. Roberts, Roger W. Romani, C. Sgrò, Patrick Slane, P. Soffitta, G. Spandre, Douglas A. Swartz, Toru Tamagawa, F. Tavecchio, Yuzuru Tawara, Allyn F. Tennant, Nicholas E. Thomas, Francesco Tombesi, A. Trois, R. Turolla, Jacco VinkList of authors in order
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https://doi.org/10.1051/0004-6361/202450937Publisher landing page
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YesWhether a free full text is available
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hybridOpen access status per OpenAlex
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https://doi.org/10.1051/0004-6361/202450937Direct OA link when available
- Concepts
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Physics, Astrophysics, Pulsar, Astronomy, X-ray, OpticsTop concepts (fields/topics) attached by OpenAlex
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12Total citation count in OpenAlex
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2025: 10, 2024: 2Per-year citation counts (last 5 years)
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50Number of works referenced by this work
- Related works (count)
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.evolution | 250 |
| abstract_inverted_index.intricate | 21 |
| abstract_inverted_index.performed | 6 |
| abstract_inverted_index.∼100°. | 213 |
| abstract_inverted_index.Scattering | 265 |
| abstract_inverted_index.decreasing | 169 |
| abstract_inverted_index.decrements | 176 |
| abstract_inverted_index.displaying | 58 |
| abstract_inverted_index.high-state | 287 |
| abstract_inverted_index.individual | 240 |
| abstract_inverted_index.luminosity | 80 |
| abstract_inverted_index.precessing | 271 |
| abstract_inverted_index.properties | 237, 283 |
| abstract_inverted_index.pulsar’s | 235 |
| abstract_inverted_index.supporting | 253 |
| abstract_inverted_index.Observation | 135, 144, 154 |
| abstract_inverted_index.Polarimetry | 11 |
| abstract_inverted_index.constraints | 232 |
| abstract_inverted_index.geometrical | 236 |
| abstract_inverted_index.investigate | 19 |
| abstract_inverted_index.luminosity, | 170 |
| abstract_inverted_index.pulse-phase | 215 |
| abstract_inverted_index.responsible | 276 |
| abstract_inverted_index.significant | 109, 184 |
| abstract_inverted_index.observations | 1, 46 |
| abstract_inverted_index.polarimetric | 282 |
| abstract_inverted_index.polarimetry. | 37 |
| abstract_inverted_index.polarization | 110, 120, 124, 187 |
| abstract_inverted_index.variability. | 60 |
| abstract_inverted_index.corresponding | 205 |
| abstract_inverted_index.observations, | 114 |
| abstract_inverted_index.observations. | 241 |
| abstract_inverted_index.super-orbital | 59, 76, 263, 291 |
| abstract_inverted_index.phase-averaged | 119 |
| abstract_inverted_index.phase-resolved | 180 |
| abstract_inverted_index.anti-correlation | 221 |
| abstract_inverted_index.spectro-polarimetric | 158, 181 |
| cited_by_percentile_year.max | 99 |
| cited_by_percentile_year.min | 94 |
| countries_distinct_count | 0 |
| institutions_distinct_count | 104 |
| citation_normalized_percentile.value | 0.95970562 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | True |