NEARBY GALAXIES
Overview of the SDSS IV MaNGA survey: mapping nearby galaxies at Apache Point Observatory
... (SDSS-IV) that began on 2014 July 1. MaNGA will investigate the internal kinematic structure and composition of gas and stars in an unprecedented sample of 10,000 nearby galaxies. We summarize essential ...
24
DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet microwave bands
... in nearby galaxies (and to do so across the very di ff erent resolutions and noise environments found in mul- tiwavelength ...for nearby galaxies, which are often “shredded” ...of ...
31
PAHs and star formation in the H II regions of nearby galaxies M83 and M33
... host galaxies of these H ii regions span a range of metallicites, SFR, and stellar masses, and their basic properties are summarized in Table ...Infrared Nearby Galaxies Sur- vey (SINGS) galaxy ...
26
Sloan Digital Sky Survey IV: mapping the Milky Way, nearby galaxies, and the distant universe
... Mapping Nearby Galaxies at Apache Point Observatory ( MaNGA ) survey is obtaining spatially resolved spectroscopy for thousands of nearby galaxies ( median z ~ ...and galaxies in X-ray ...
35
The Ionized Gas in Nearby Galaxies as Traced by the [N II] 122 and 205 μm Transitions
... of nearby galaxies ( ...star-forming galaxies and ( U ) LIRGs by Farrah et ...star-forming galaxies with infrared luminosities below ∼ 10 ...luminous galaxies, these calibrations tend ...
17
Overview of the SDSS IV MaNGA survey : mapping nearby galaxies at Apache Point Observatory
... of galaxies, but also revealed how the star formation rates (SFRs), metallic- ities, stellar populations, morphologies, and black hole growth rates of galaxies vary with mass, environment, and ...
26
Massive Black Holes in Nearby Galaxies
... EXPECTED FREQUENCY AND MASSES OF DEAD QUASARS We may estimate the density of the mass p of the total luminosity released by quasars during the history of the universe from the observed c[r] ...
6
MaNGA: Mapping Nearby Galaxies at Apache Point Observatory
... the galaxies in the P-MaNGA ...spheroidal galaxies, while in late-type galaxies the metallicity gradient is flat and the age gradient is negative, consistent with current literature ...
7
Gallazzi, Anna (2006): Modeling and interpretation of galaxy spectra: the stellar populations of nearby galaxies. Dissertation, LMU München: Fakultät für Physik
... of galaxies with an accuracy better than ...the galaxies in the ...the galaxies with the strongest absorption features, that have a smooth, continuous star formation ...to galaxies with S/N ...
193
On the M σ Relationship and SMBH Mass Estimates of Selected Nearby Galaxies
... of galaxies: 12 ellipticals, 2 probable ellipticals, 13 barred spirals, 12 spirals, an ir- regular and some cross-type ...elliptical galaxies was ...
9
Bulges and Disks in the Nearby Universe: Applications to Evolution and Formation of Galaxies
... base. Galaxies that satisfy three main selection criteria were ...large, nearby galaxies that are typically either too well resolved to be fitted with a standard smooth light profile or shredded into ...
340
Predicted MOND velocity dispersions for a catalog of ultra diffuse galaxies in group environments
... elliptical galaxies – NGC 5485 and NGC 5473 with similar mass estimates – at a distance of 27 ...other nearby galaxies NGC 5475 and NGC 5443, ...two galaxies have the same systemic velocity ...
9
Gemini NIFS survey of feeding and feedback processes in nearby active galaxies - II. The sample and surface mass density profiles
... Emission lines from high, low-ionization and molecu- lar gas, as well as strong CO absorptions, are usually ob- served at these spectral bands in spectra of active galax- ies (e.g. Riffel, Rodr´ıguez-Ardila & ...
18
Monsters on the Move: Gravitational Recoil of Supermassive Black Holes in Nearby Elliptical Galaxies
... 14 nearby elliptical core galaxies for their ...of galaxies used in Lena et ...of nearby early-type ...elliptical galaxies in their sample but we expanded our sample to include both ...
148
Grimm, Hans-Jakob (2003): X-ray binaries in the Milky Way and other galaxies. Dissertation, LMU München: Fakultät für Physik
... of galaxies, each having a population of such sources, the most probable value of the integrated luminosity of an arbitrarily chosen galaxy (the mode of the distribution) equals to the mean luminosity (averaged ...
128
Barden, Marco (2004): The Evolution of the Tully-Fisher Relation at Redshift z~1. Dissertation, LMU München: Fakultät für Physik
... observed galaxies from the literature are a factor of two smaller than ours (see ...target galaxies than true ...brightest galaxies at intermediate redshift would be over a magnitude fainter as in ...
238
The ESO Nearby Abell Cluster Survey. XIII. The orbits of the different types of galaxies in rich clusters
... the galaxies must be in the tangential ...the galaxies of di ff erent morphological types was only half that which is ...the galaxies of dif- ferent types, and not just different energy ...the ...
13
The ESO nearby Abell cluster survey. VII. Galaxy density profiles of rich clusters of galaxies
... -18.4) galaxies. We conclude that the brighter galaxies are represented almost equally well by King and NFW profiles, but that the distribution of the fainter galaxies clearly shows a core rather ...
20
The ESO Nearby Abell Cluster Survey. VI. Spatial distribution and kinematics of early- and late-type galaxies
... type galaxies would be larger than the apparent ...late-type galaxies in the main concentration of the Coma cluster is very close to √ 2 times that of the early-type ...
14