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Letter
Nature 455, 506-509 (25 September 2008) | doi:10.1038/nature07328; Received 31 January 2008; Accepted 31 July 2008
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Flares from a candidate Galactic magnetar suggest a missing link to dim isolated neutron stars
A. J. Castro-Tirado1, A. de Ugarte Postigo1,2, J. Gorosabel1, M. Jelínek1, T. A. Fatkhullin3, V. V. Sokolov3, P. Ferrero4, D. A. Kann4, S. Klose4, D. Sluse5, M. Bremer6, J. M. Winters6, D. Nuernberger2, D. Pérez-Ramírez7,8, M. A. Guerrero1, J. French9, G. Melady9, L. Hanlon9, B. McBreen9, K. Leventis10, S. B. Markoff10, S. Leon11, A. Kraus12, F. J. Aceituno1, R. Cunniffe1,13, P. Kubánek1,14, S. Vítek1, S. Schulze4, A. C. Wilson15, R. Hudec16, M. Durant17, J. M. González-Pérez17, T. Shahbaz17, S. Guziy18, S. B. Pandey19, L. Pavlenko20, E. Sonbas3,21, S. A. Trushkin3, N. N. Bursov3, N. A. Nizhelskij3, C. Sánchez-Fernández22 & L. Sabau-Graziati23
- Instituto de Astrofísica de Andalucía del Consejo Superior de Investigaciones Científicas (IAA-CSIC), PO Box 03004, E-18080 Granada, Spain
- European Southern Observatory, Casilla 19001, Santiago 19, Chile
- Special Astrophysical Observatory of Russian Academy of Science (SAO-RAS), Nizhnij Arkhyz, Karachai-Cherkessia, 369167 Russia
- Thüringer Landessternwarte Tautenburg, Sternwarte 5, D-07778 Tautenburg, Germany
- Laboratoire d'Astrophysique, École Polytechnique Fédérale de Lausanne (EPFL) Observatoire, 1290 Sauverny, Switzerland
- Institute de Radioastronomie Millimétrique (IRAM), 300 rue de la Piscine, 38406 Saint Martin d'Héres, France
- Facultad de Ciencias Experimentales, Universidad de Jaén, Campus Las Lagunillas, E-23071 Jaén, Spain
- Department of Physics and Astronomy, The University of Leicester, Leicester, LE1 7RH, UK
- School of Physics, University College Dublin, Dublin 4, Ireland
- Astronomical Institute 'Anton Pannekoek', University of Amsterdam, 1098 SJ Amsterdam, The Netherlands
- Institute de Radioastronomie Millimétrique (IRAM), Avda. Divina Pastora 7, Núcleo Central, E-18012 Granada, Spain
- Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
- Cork Institute of Technology, Rossa Avenue, Bishopstown (Cork), Ireland
- Universidad de Valencia, Edif. Institutos de Investigación (GACE-ICMOL), Campus de Paterna, E-46980 Paterna (Valencia), Spain
- Department of Astronomy, University of Texas, Austin, Texas 78712, USA
- Astronomical Institute of the Czech Academy of Sciences, Fri
ova 298, 25165 Ond
ejov, Czech Republic - Instituto de Astrofísica de Canarias (IAC), Via Láctea s/n, E-38205 La Laguna (Tenerife), Spain
- Nikolaev State University, Nikolskaya 24, 54030 Nikolaev, Ukraine
- Aryabhatta Research Institute of Observational-Sciences (ARIES), Manora Peak, NainiTal, Uttarakhand, 263129, India
- Crimean Astrophysical Observatory, 98409 Nauchny, Ukraine
- University of Cukurova, Department of Physics, 01330 Adana, Turkey
- European Space Astronomy Centre (ESAC), Avenida de los Castillos s/n, Urbanizacion Villafranca del Castillo, E-28691 Villanueva de la Cañada (Madrid), Spain
- Instituto Nacional de Técnica Aeroespacial (INTA), E-28750 Torrejón de Ardoz (Madrid), Spain
Correspondence to: A. J. Castro-Tirado1 Correspondence and requests for materials should be addressed to A.J.C.T. (Email: ajct@iaa.es).
Abstract
Magnetars1 are young neutron stars with very strong magnetic fields of the order of 1014–1015 G. They are detected in our Galaxy either as soft
-ray repeaters or anomalous X-ray pulsars. Soft
-ray repeaters are a rare type of
-ray transient sources that are occasionally detected as bursters in the high-energy sky2, 3, 4. No optical counterpart to the
-ray flares or the quiescent source has yet been identified. Here we report multi-wavelength observations of a puzzling source, SWIFT J195509+261406. We detected more than 40 flaring episodes in the optical band over a time span of three days, and a faint infrared flare 11 days later, after which the source returned to quiescence. Our radio observations confirm a Galactic nature and establish a lower distance limit of
3.7 kpc. We suggest that SWIFT J195509+261406 could be an isolated magnetar whose bursting activity has been detected at optical wavelengths, and for which the long-term X-ray emission is short-lived. In this case, a new manifestation of magnetar activity has been recorded and we can consider SWIFT J195509+261406 to be a link between the 'persistent' soft
-ray repeaters/anomalous X-ray pulsars and dim isolated neutron stars.
- Instituto de Astrofísica de Andalucía del Consejo Superior de Investigaciones Científicas (IAA-CSIC), PO Box 03004, E-18080 Granada, Spain
- European Southern Observatory, Casilla 19001, Santiago 19, Chile
- Special Astrophysical Observatory of Russian Academy of Science (SAO-RAS), Nizhnij Arkhyz, Karachai-Cherkessia, 369167 Russia
- Thüringer Landessternwarte Tautenburg, Sternwarte 5, D-07778 Tautenburg, Germany
- Laboratoire d'Astrophysique, École Polytechnique Fédérale de Lausanne (EPFL) Observatoire, 1290 Sauverny, Switzerland
- Institute de Radioastronomie Millimétrique (IRAM), 300 rue de la Piscine, 38406 Saint Martin d'Héres, France
- Facultad de Ciencias Experimentales, Universidad de Jaén, Campus Las Lagunillas, E-23071 Jaén, Spain
- Department of Physics and Astronomy, The University of Leicester, Leicester, LE1 7RH, UK
- School of Physics, University College Dublin, Dublin 4, Ireland
- Astronomical Institute 'Anton Pannekoek', University of Amsterdam, 1098 SJ Amsterdam, The Netherlands
- Institute de Radioastronomie Millimétrique (IRAM), Avda. Divina Pastora 7, Núcleo Central, E-18012 Granada, Spain
- Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
- Cork Institute of Technology, Rossa Avenue, Bishopstown (Cork), Ireland
- Universidad de Valencia, Edif. Institutos de Investigación (GACE-ICMOL), Campus de Paterna, E-46980 Paterna (Valencia), Spain
- Department of Astronomy, University of Texas, Austin, Texas 78712, USA
- Astronomical Institute of the Czech Academy of Sciences, Fri
ova 298, 25165 Ond
ejov, Czech Republic - Instituto de Astrofísica de Canarias (IAC), Via Láctea s/n, E-38205 La Laguna (Tenerife), Spain
- Nikolaev State University, Nikolskaya 24, 54030 Nikolaev, Ukraine
- Aryabhatta Research Institute of Observational-Sciences (ARIES), Manora Peak, NainiTal, Uttarakhand, 263129, India
- Crimean Astrophysical Observatory, 98409 Nauchny, Ukraine
- University of Cukurova, Department of Physics, 01330 Adana, Turkey
- European Space Astronomy Centre (ESAC), Avenida de los Castillos s/n, Urbanizacion Villafranca del Castillo, E-28691 Villanueva de la Cañada (Madrid), Spain
- Instituto Nacional de Técnica Aeroespacial (INTA), E-28750 Torrejón de Ardoz (Madrid), Spain
Correspondence to: A. J. Castro-Tirado1 Correspondence and requests for materials should be addressed to A.J.C.T. (Email: ajct@iaa.es).
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