Quantitative Morphology of E / s0 Galaxies - Part Two - Possible Environmental Effects on the Properties of Lenticular Galaxies

Details Quantitative Morphology of E / s0 Galaxies - Part Two - Possible Environmental Effects on the Properties of Lenticular Galaxies Quantitative Morphology of E / s0 Galaxies - Part Two - Possible Environmental Effects on the Properties of Lenticular Galaxies

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...283..779m&link_type=abstract

Astronomy and Astrophysics, Vol. 283, NO. 3/MAR(III), P. 779, 1994

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

In Paper I of this series (Michard & Marchal 1993) "E-like S0s" were defined as objects without ring nor lens, and with the disk fully embedded in a spheroidal halo. It was tentatively suggested that such objects might be comparatively more frequent in the Virgo cluster than in the general field, as is known to be the case for ellipticals. This question is reconsidered with an enlarged set of S0s (now nearly complete) and a much enlarged (and now complete) Virgo subset: the previous suggestion is confirmed.

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