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Vel. Distribution of low-luminosity E galaxies
The shape of the line-of-sight velocity distribution (LOSVD) is measured for a sample of 14 elliptical galaxies, predominantly low-luminosity ellipticals. The sample is... -
Compilation of black hole, bulge and stellar masses
We present a multiwavelength study of the active galactic nucleus in the nearby (D=14.1Mpc) low-mass galaxy IC750, which has circumnuclear 22GHz water maser emission. The masers... -
KiDS ultracompact massive galaxies sp. obs.
Ultracompact massive galaxies (UCMGs), i.e., galaxies with stellar masses M_>8x10^10^M{sun} and effective radii R_e<1.5kpc, are very rare systems, in particular at low and... -
HI and CO observations of M33 interstellar medium
We utilize the multi-wavelength data of M33 to study the origin of turbulence in its interstellar medium. We find that the HI turbulent energy surface density inside 8kpc is... -
Double-peaked narrow lines in AGN. IV. Mergers
Double-peaked narrow emission lines in active galactic nucleus (AGN) spectra can be produced by AGN outflows, rotation, or dual AGNs, which are AGN pairs in ongoing galaxy... -
Low-rotating elliptical galaxies in MaNGA
Pressure-supported systems modeled under Modified Newtonian dynamics (MOND)ian extended gravity are expected to show an outer flattening in their velocity dispersion profiles. A... -
Cloud-scale molecular gas properties in 15 galaxies
We measure the velocity dispersion, {sigma}, and surface density, {Sigma}, of the molecular gas in nearby galaxies from CO spectral line cubes with spatial resolution 45-120pc,... -
Mass-to-light ratios in low-mass early-type gal.
We present dynamical measurements of the central mass-to-light ratio (M/L) of a sample of 27 low-mass early-type ATLAS^3D^ galaxies. We consider all ATLAS^3D^ galaxies with... -
Star forming cloud-giant molecular cloud complexes
Star formation on galactic scales is known to be a slow process, but whether it is slow on smaller scales is uncertain. We cross-correlate 5469 giant molecular clouds (GMCs)... -
Group of galaxies in gravitational lens fields
With a large, unique spectroscopic survey in the fields of 28 galaxy-scale strong gravitational lenses, we identify groups of galaxies in the 26 adequately sampled fields. Using... -
Galactic MCs associated with HII regions
The relations between star formation and properties of molecular clouds (MCs) are studied based on a sample of star-forming regions in the Galactic Plane. Sources were selected... -
HSTPROMO catalogs of GCs. IV. Blue straggler stars
We make use of the Hubble Space Telescope proper-motion catalogs derived by Bellini et al. (Paper I, 2014, J/ApJ/797/115) to produce the first radial velocity dispersion... -
A new reverberation mapping campaign on NGC 5548
NGC 5548 is the best-observed reverberation-mapped active galactic nucleus with long-term, intensive monitoring. Here we report results from a new observational campaign between... -
SDSS-DR7 broad-line QSOs
The diverse properties of broad-line quasars appear to follow a well-defined main sequence along which the optical FeII strength increases. It has been suggested that this... -
Masses of giant molecular clouds in Milky Way
The mass fraction of dense gas within giant molecular clouds (GMCs) of the Milky Way is investigated using ^13^CO data from the Five College Radio Astronomy Observatory Galactic... -
Molecular clouds in the Antennae from CO(2-1)
Super star clusters--extremely massive clusters found predominately in starburst environments--are essential building blocks in the formation of galaxies and thought to dominate... -
Dispersion-supported stellar systems
We examine scaling relations of dispersion-supported galaxies over more than eight orders of magnitude in luminosity by transforming standard fundamental plane parameters into a... -
Velocities in Cl 0024+16 and MS 0451-03
We examine resolved spectroscopic data obtained with the Keck II telescope for 44 spheroidal galaxies in the fields of two rich clusters, Cl 0024+16 (z=0.40) and MS 0451-03... -
Cusp radius in luminous elliptical galaxies
Black hole (BH) masses predicted from the M_BH_-sigma relationship conflict with predictions from the M_BH_-L relationship for high-luminosity galaxies, such as brightest... -
Velocity dispersion in AGN
It has been proposed that the width of the narrow [O III] {lambda}5007 emission line can be used as a surrogate for the stellar velocity dispersion in active galaxies. This...
