Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …

▪ Abstract Observations of star formation rates (SFRs) in galaxies provide vital clues to the
physical nature of the Hubble sequence and are key probes of the evolutionary histories of …

Fast radio bursts (FRBs) are brief, bright, extragalactic radio flashes,. Their physical origin
remains unknown, but dozens of possible models have been postulated. Some FRB sources …

The precise localization of the repeating fast radio burst (FRB 121102) has provided the first
unambiguous association (chance coincidence probability p≲ 3× 10− 4) of an FRB with an …

We review recent determinations of the present‐day mass function (PDMF) and initial mass
function (IMF) in various components of the Galaxy—disk, spheroid, young, and globular …

Measurements of H α, HI, and CO distributions in 61 normal spiral galaxies are combined
with published far-infrared and CO observations of 36 infrared-selected starburst galaxies, in …

We present a comprehensive study of the physical properties of∼ 105 galaxies with
measurable star formation in the Sloan Digital Sky Survey (SDSS). By comparing physical …

We present new calibrations of far-ultraviolet (FUV) attenuation as derived from the total
infrared to FUV luminosity ratio (IRX) and the FUV–near-UV (NUV) color. We find that the …

Template fits to observed galaxy fluxes allow calculation of K-corrections and conversions
among observations of galaxies at various wavelengths. We present a method for creating …

Strong constraints on the cosmic star formation history (SFH) have recently been established
using ultraviolet and far-infrared measurements, refining the results of numerous …