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Emission Line Regions in M86

Published online by Cambridge University Press:  25 May 2016

S. Döbereiner ,
J. Heidt  and
S. J. Wagner
S. Döbereiner
Affiliation:
Max-Planck Institut für Extraterrestrische Physik, Garching, Germany
J. Heidt
Affiliation:
Landessternwarte Heidelberg, Germany
S. J. Wagner
Affiliation:
Landessternwarte Heidelberg, Germany

Extract

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We present broad- and narrow-band (B, R, Hα+[NII] and Hα 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.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 364
Copyright
Copyright © Kluwer 1996