Abstract
We present broad- and narrow-band (B, R, Hα+[NII] and Ha continuum) observations of M86 obtained with a focal reducer at the Calar Alto 1.23m telescope, to look for any signs of material cooling out from the hot X-ray emitting ISM. The above figures show a quotient image (13’ × 13’, north up) (Hα cont. — Hα) to the left, and a Hα image (right) from which the light of the stellar spheroid of M86 has been subtracted. Both are overlayed with ROSAT PSPC X-ray contours.
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© 1996 Springer Science+Business Media Dordrecht
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Döbereiner, S., Heidt, J., Wagner, S.J. (1996). Emission Line Regions in M86. In: Bender, R., Davies, R.L. (eds) New Light on Galaxy Evolution. International Astronomical Union / Union Astronomique Internationale, vol 171. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0229-9_76
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DOI: https://doi.org/10.1007/978-94-009-0229-9_76
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-3976-2
Online ISBN: 978-94-009-0229-9
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