Understanding the LMXB X2127+119 in M 15. II. The UV data

Z. Ioannou, L. Van Zyl, T. Naylor, P. A. Charles, B. Margon, L. Koch-Miramond, S. Ilovaisky

Research output: Contribution to journalArticle

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Abstract

We present HST UV observations of the high-inclination low mass X-ray binary AC211 (X2127+119), which is located in the globular cluster M 15 (NGC 7078). We have discovered a CIV P Cygni profile in this system, which confirms the existence of an outflow from AC211. The outflow velocity as measured from the P Cygni profile is ≃ 1500 km s-1. We calculate that the mass lost through this wind is too small to support a large period derivative as favoured by Homer & Charles (1998). Using new X-ray observations we have revised the ephemeris for AC211 and we find no evidence in support of a period derivative. The UV spectrum exhibits several absorption features due to O, Si and C. The very strong HeII line at 1640 Å is not seen to modulate strongly with orbital phase, suggesting its origin lies in the outer parts of the system. In contrast, the eclipse of the UV continuum is short compared with the X-ray and optical eclipses.

Original languageEnglish
Pages (from-to)211-218
Number of pages8
JournalAstronomy and Astrophysics
Volume399
Issue number1
Publication statusPublished - Feb 2003

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eclipses
outflow
x rays
profiles
globular clusters
inclination
continuums
orbitals

Keywords

  • Accretion, accretion discs
  • Stars: binaries: eclipsing
  • Stars: coronae
  • Stars: individual: X2127+119, AC211
  • Ultraviolet: stars

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Ioannou, Z., Van Zyl, L., Naylor, T., Charles, P. A., Margon, B., Koch-Miramond, L., & Ilovaisky, S. (2003). Understanding the LMXB X2127+119 in M 15. II. The UV data. Astronomy and Astrophysics, 399(1), 211-218.

Understanding the LMXB X2127+119 in M 15. II. The UV data. / Ioannou, Z.; Van Zyl, L.; Naylor, T.; Charles, P. A.; Margon, B.; Koch-Miramond, L.; Ilovaisky, S.

In: Astronomy and Astrophysics, Vol. 399, No. 1, 02.2003, p. 211-218.

Research output: Contribution to journalArticle

Ioannou, Z, Van Zyl, L, Naylor, T, Charles, PA, Margon, B, Koch-Miramond, L & Ilovaisky, S 2003, 'Understanding the LMXB X2127+119 in M 15. II. The UV data', Astronomy and Astrophysics, vol. 399, no. 1, pp. 211-218.
Ioannou Z, Van Zyl L, Naylor T, Charles PA, Margon B, Koch-Miramond L et al. Understanding the LMXB X2127+119 in M 15. II. The UV data. Astronomy and Astrophysics. 2003 Feb;399(1):211-218.
Ioannou, Z. ; Van Zyl, L. ; Naylor, T. ; Charles, P. A. ; Margon, B. ; Koch-Miramond, L. ; Ilovaisky, S. / Understanding the LMXB X2127+119 in M 15. II. The UV data. In: Astronomy and Astrophysics. 2003 ; Vol. 399, No. 1. pp. 211-218.
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