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NGC 1624-2: a slowly rotating, X-ray luminous Of?cp star with an extraordinarily strong magnetic field†

  1. G. A. Wade1,*,
  2. J. Maíz Apellániz2,
  3. F. Martins3,
  4. V. Petit4,
  5. J. Grunhut1,
  6. N. R. Walborn5,
  7. R. H. Barbá6,
  8. M. Gagné4,
  9. E. García-Melendo7,8,
  10. J. Jose9,
  11. A. F. J. Moffat10,
  12. Y. Nazé11,
  13. C. Neiner12,
  14. A. Pellerin13,
  15. M. Penadés Ordaz2,
  16. M. Shultz1,
  17. S. Simón-Díaz14,
  18. A. Sota2,
  19. the MiMeS Collaboration

Article first published online: 3 AUG 2012

DOI: 10.1111/j.1365-2966.2012.21523.x

Issue

Monthly Notices of the Royal Astronomical Society

Monthly Notices of the Royal Astronomical Society

Volume 425, Issue 2, pages 1278–1293, 11 September 2012

Additional Information

How to Cite

Wade, G. A., Apellániz, J. M., Martins, F., Petit, V., Grunhut, J., Walborn, N. R., Barbá, R. H., Gagné, M., García-Melendo, E., Jose, J., Moffat, A. F. J., Nazé, Y., Neiner, C., Pellerin, A., Ordaz, M. P., Shultz, M., Simón-Díaz, S., Sota, A. and the MiMeS Collaboration (2012), NGC 1624-2: a slowly rotating, X-ray luminous Of?cp star with an extraordinarily strong magnetic field. Monthly Notices of the Royal Astronomical Society, 425: 1278–1293. doi: 10.1111/j.1365-2966.2012.21523.x

Author Information

  1. 1

    Department of Physics, Royal Military College of Canada, Kingston, Ontario, Canada

  2. 2

    Instituto de Astrofísica de Andalucía–CSIC, Granada, Spain

  3. 3

    LUPM-UMR5299, CNRS & Université Montpellier II, Montpellier, France

  4. 4

    Department of Geology & Astronomy, West Chester University, West Chester, PA, USA

  5. 5

    Space Telescope Science Institute, Baltimore, MD, USA

  6. 6

    Instituto de Ciencias Astronómicas, San Juan, Argentina

  7. 7

    Fundació Privada Observatori Esteve Duran, Seva, Barcelona, Spain

  8. 8

    Institut de Ciències de l’Espai (CSIC-IEEC), Campus UAB, Bellaterra, Spain

  9. 9

    Indian Institute of Astrophysics, Bangalore, India

  10. 10

    Département de physique, Université de Montréal, Montréal, QC, Canada

  11. 11

    FNRS–GAPHE, Département AGO, Université de Liège, B4000-Liège, Belgium

  12. 12

    LESIA, UMR 8109 du CNRS, Observatoire de Paris, UPMC, Université Paris Diderot, Meudon Cedex, France

  13. 13

    Department of Physics and Astronomy, Texas A&M University, TX, USA

  14. 14

    Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain

*E-mail: wade-g@rmc.ca

  1. †

    Based on spectropolarimetric observations obtained at the Canada–France–Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l’Univers (INSU) of the Centre National de la Recherche Scientifique of France, and the University of Hawaii, as well as on observations obtained using the Narval spectropolarimeter at the Observatoire du Pic du Midi (France), which is operated by the INSU. The spectroscopic data were gathered with five facilities: the 9.2-m Hobby–Eberly Telescope at McDonald Observatory (MDO), the 3.5-m Telescope at Calar Alto Observatory (CAHA), the 1.5-m Telescope at the Observatorio de Sierra Nevada (OSN), the 4.2-m William Herschel Telescope at the Observatorio del Roque de los Muchachos (ORM) and the 2-m Himalayan Chandra Telescope at Indian Astronomical Observatory (IAO).

Publication History

  1. Issue published online: 22 AUG 2012
  2. Article first published online: 3 AUG 2012
  3. Manuscript Accepted: 13 JUN 2012
  4. Manuscript Received: 13 JUN 2012

Funded by

  • Natural Science and Engineering Research Council of Canada (NSERC)
  • Spanish Ministerio de Ciencia e Innovación. Grant Numbers: AYA2010-15081, AYA2010-17631
  • Junta de Andalucía. Grant Number: P08-TIC-4075
  • George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy
  • Fonds National de la Recherche Scientifique (Belgium)
  • Communauté Frana¸ise de Belgique
  • PRODEX XMM and Integral contracts
  • Action de Recherche Concertée (CFWB–Académie Wallonie Europe)
  • Fonds Québecois de la Recherche sur la Nature et les Technologies

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