Detection of a temperature structure in the coma cluster of galaxies with ASCA

H. Honda, M. Hirayama, M. Watanabe, H. Kunieda, Y. Tawara, K. Yamashita, T. Ohashi, John Hughes, J. P. Henry

Research output: Contribution to journalArticle

63 Scopus citations

Abstract

Significant temperature variation is found from ASCA observations of the hot intracluster medium in the Coma cluster of galaxies. The whole cluster out to 1° from the center was covered by 14 pointings. The temperature of the hot gas in the outside region is estimated by correcting for the stray-light effect from the bright center. The inferred temperature is lower than 4.5 keV in the west region and higher than 10 keV in the east, both offset by 40' (1.6 Mpc for H0 = 50 km s-1 Mpc-1) from the center. The temperature variation is not explained by a systematic error in the complex point-spread function of the ASCA X-ray telescope. The azimuthal variation of temperature is probably caused by recent mergers and may reflect an extended distribution of the dark matter.

Original languageEnglish (US)
Pages (from-to)L71-L74
JournalAstrophysical Journal
Volume473
Issue number2 PART II
StatePublished - Jan 1 1996

    Fingerprint

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Galaxies: clusters: individual (Coma)
  • Galaxies: intergalactic medium
  • X-rays: galaxies

Cite this

Honda, H., Hirayama, M., Watanabe, M., Kunieda, H., Tawara, Y., Yamashita, K., Ohashi, T., Hughes, J., & Henry, J. P. (1996). Detection of a temperature structure in the coma cluster of galaxies with ASCA. Astrophysical Journal, 473(2 PART II), L71-L74.