This paper reviews surface photometry of bulges and elliptical galaxies. Work prior to 1982
is discussed by Kormendy (1982). Since then, the subject has gone through a revolution …

Theories of how galaxies, the fundamental constituents of large-scale structure, form and
evolve have undergone a dramatic paradigm shift in the last few decades. Earlier views …

We present evidence that ripples (" shells") occur not only in ellipticals, as hitherto believed,
but also in disk galaxies of Hubble types S0, S0/Sa, and Sa, and probably even in the Sbc …

envelope luminosity and cluster properties (richness, cluster X-ray luminosity, Bautz-Morgan
type, and RoodSastry type) substantiate arguments for the dynamical formation of …

NGC 4449 is a nearby Magellanic irregular starburst galaxy with a B-band absolute
magnitude of− 18 and a prominent, massive, intermediate-age nucleus at a distance from …

A multicolor photometric study of the tidal features in interacting galaxies ADS Classic is now
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …

We present deep, wide-field imaging of the M96 galaxy group (also known as the Leo I
Group). Down to surface brightness limits of μ B= 30.1 and μ V= 29.5, we find no diffuse …

Context. Shells in Elliptical Galaxies are faint, sharp-edged features, believed to provide
evidence for a merger event. Accurate photometry at high spatial resolution is needed to …

We have conducted a BVR imaging survey of nine early-type galaxies previously verified to
exist in extremely isolated environments. Our goals are to establish a baseline of …

We have used the VLA B and C Arrays to make 21 cm HI observations of the peculiar galaxy
NGC 2782 (Arp 215). These observations are complementary to previously published D …