Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· Full Refereed Journal Article (PDF/Postscript)
· arXiv e-print (arXiv:astro-ph/0304088)
· On-line Data
· References in the article
· Citations to the Article (70) (Citation History)
· Refereed Citations to the Article
· SIMBAD Objects (3)
· Also-Read Articles (Reads History)
· HEP/Spires Information
·
· Translate This Page
Title:
A broad absorption feature in the X-ray spectrum of the isolated neutron star RBS1223 (1RXS J130848.6+212708)
Authors:
Haberl, F.; Schwope, A. D.; Hambaryan, V.; Hasinger, G.; Motch, C.
Affiliation:
AA(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching, Germany), AB(Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany), AC(Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany), AD(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching, Germany), AE(Observatoire Astronomique, UA 1280 CNRS, 11 rue de l'Université, 67000 Strasbourg, France)
Publication:
Astronomy and Astrophysics, v.403, p.L19-L23 (2003) (A&A Homepage)
Publication Date:
05/2003
Origin:
A&A
A&A Keywords:
stars: individual: RBS1223 = 1RXS J130848.6+212708, stars: neutron, stars: magnetic fields, X-rays: stars
DOI:
10.1051/0004-6361:20030450
Bibliographic Code:
2003A&A...403L..19H

Abstract

X-ray spectra of the isolated neutron star RBS1223 obtained with the instruments on board XMM-Newton in December 2001 and January 2003 show deviations from a Planckian energy distribution at energies below 500 eV. The spectra are well fit when a broad, Gaussian-shaped absorption line with sigma = 100 eV and centered at an energy of 300 eV is added to an absorbed blackbody model. The resulting equivalent width of the line is -150 eV. However, the spectral resolution at these low energies of the EPIC detectors and the lower statistical quality and restricted energy band of the RGS instruments are not sufficient to exclude even broader lines at energies down to 100 eV or several unresolved lines. The most likely interpretation of the absorption feature is a cyclotron absorption line produced by protons in the magnetic field of the neutron star. In this picture line energies of 100-300 eV yield a magnetic field strength of 2-613 G for a neutron star with canonical mass and radius. Folding light curves from different energy bands at a period of 10.31 s, which implies a double peaked pulse profile, shows different hardness ratios for the two peaks. This confirms that the true spin period of RBS1223 is twice as long as originally thought and suggests variations in cyclotron absorption with pulse phase. We also propose that changes in photo-electric absorption seen in phase resolved spectra of RX J0720.4-3125 by Cropper et al. (\cite{2001A&A...365L.302C), when formally fit with an absorbed blackbody model, are caused instead by cyclotron absorption varying with pulse phase.

Based on observations with XMM-Newton, an ESA Science Mission with instruments and contributions directly funded by ESA Member states and the USA (NASA).

Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)
   

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints