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Near-IR Imaging Spectroscopy of CD Galaxy NGC1275

Published online by Cambridge University Press:  25 May 2016

B. J. Sams ,
R. Genzel ,
A. Krabbe ,
N. Thatte  and
H. Kroker
B. J. Sams
Affiliation:
Max Planck Institut für extraterrestrische Physik, Giessenbachstrasse 85748 Garching, GERMANY
R. Genzel
Affiliation:
Max Planck Institut für extraterrestrische Physik, Giessenbachstrasse 85748 Garching, GERMANY
A. Krabbe
Affiliation:
Max Planck Institut für extraterrestrische Physik, Giessenbachstrasse 85748 Garching, GERMANY
N. Thatte
Affiliation:
Max Planck Institut für extraterrestrische Physik, Giessenbachstrasse 85748 Garching, GERMANY
H. Kroker
Affiliation:
Max Planck Institut für extraterrestrische Physik, Giessenbachstrasse 85748 Garching, GERMANY

Extract

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H and K band imaging spectroscopy of the central 12″ (4.2 kpc) of NGC1275 using the Max-Planck-Institut für extraterrestrische Physik imaging spectrometer “3D” maps the gas density and temperature in the core and separates the contribution of Seyfert emission to the core light.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 440
Copyright
Copyright © Kluwer 1996