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NGC 3077: Hα Features and the Young Population

Published online by Cambridge University Press:  25 May 2016

H. Abdel-Hamid  and
P. Notni
H. Abdel-Hamid
Affiliation:
Astrophysikalisches Institut Potsdam, D-14482 Potsdam, Germany
P. Notni
Affiliation:
Astrophysikalisches Institut Potsdam, D-14482 Potsdam, Germany

Extract

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NGC 3077, an Irr II galaxy in the M81/M82 group of galaxies at 3.63 Mpc, suffered a tidal encounter with M81 about 400 Myr ago. Tidal structures of HI in this group of galaxies can best be seen in a VLA image by Yun et al. (1994).

Type
IV. AGN Related Phenomena
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 439 - 441
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Abdel-Hamid, H.A. 1998, Dissertation, Uni. Potsdam, Wissensch.-verlag Berlin.Google Scholar
Hodge, P., Lee, M., & Kennicutt, R. 1989, PASP, 101, 32.Google Scholar
Miller, B.W., & Hodge, P. 1994, ApJ, 427, 656.Google Scholar
Scarrott, S.M., Rolph, C.D. & Semple, D.P. 1990, in IAU Symposium 140, 245.Google Scholar
Yun, M.S., Ho, P.T.P. & Lo, K.Y. 1994, Nature 372, 530.Google Scholar