The Origin of the Stellar Mass Distribution and Multiplicity [PDF]
Space Science Reviews, 2020 Review chapter published in Space Science ...
Yueh-Ning Lee +7 more
openaire +3 more sources
Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei [PDF]
, 2016 The Laser Interferometer Gravitational-wave Observatory (LIGO) found direct evidence for double black hole binaries emitting gravitational waves. Galactic nuclei are expected to harbor the densest population of stellar-mass black holes.
I. Bartos +3 more
semanticscholar +1 more source
Stellar mass as the ‘glocal’ driver of galaxies’ stellar population properties [PDF]
Monthly Notices of the Royal Astronomical Society, 2022 ABSTRACT The properties of the stellar populations in a galaxy are known to correlate with the amount and the distribution of stellar mass. We take advantage of the maps of light-weighted mean stellar age $\mathit {\mathrm{ Age}_{\mathrm{ wr}}}$ and metallicity $\mathit {\mathrm{ Z}_{*\mathrm{ wr}}}$ for a sample of 362 galaxies from the
Stefano Zibetti, Anna R Gallazzi
openaire +3 more sources
ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: THE INFRARED EXCESS OF UV-SELECTED z = 2–10 GALAXIES AS A FUNCTION OF UV-CONTINUUM SLOPE AND STELLAR MASS [PDF]
, 2016 We make use of deep 1.2 mm continuum observations (12.7 μJy beam−1 rms) of a 1 arcmin2 region in the Hubble Ultra Deep Field to probe dust-enshrouded star formation from 330 Lyman-break galaxies spanning the redshift range z = 2–10 (to ∼2–3 M⊙ yr−1 at 1σ
Rychard J. Bouwens +27 more
semanticscholar +1 more source
The Constant Average Relationship between Dust-obscured Star Formation and Stellar Mass from z = 0 to z = 2.5 [PDF]
, 2017 The total star formation budget of galaxies consists of the sum of the unobscured star formation, as observed in the rest-frame ultraviolet (UV), together with the obscured component that is absorbed and re-radiated by dust grains in the infrared.
K. Whitaker +5 more
semanticscholar +1 more source
Limits on Stellar-Mass Compact Objects as Dark Matter from Gravitational Lensing of Type Ia Supernovae. [PDF]
Physical Review Letters, 2017 The nature of dark matter (DM) remains unknown despite very precise knowledge of its abundance in the Universe. An alternative to new elementary particles postulates DM as made of macroscopic compact halo objects (MACHO) such as black holes formed in the
M. Zumalacárregui, U. Seljak
semanticscholar +1 more source
Simulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and luminosity functions [PDF]
, 2017 We present a suite of cosmological zoom-in simulations at z>5 from the Feedback In Realistic Environments project, spanning a halo mass range M_halo~10^8-10^12 M_sun at z=5.
Xiangcheng Ma +15 more
semanticscholar +1 more source
Mass Measurements of Stellar and Intermediate-Mass Black Holes [PDF]
Space Science Reviews, 2013 28 pages, 12 figures. Accepted for publication in Space Science Reviews (DOI 10.1007/s11214-013-0030-6). Also to appear in hard cover in the Space Sciences Series of ISSI "The Physics of Accretion onto Black Holes" (Springer Publisher).
Jorge Casares +4 more
openaire +8 more sources
Galaxy And Mass Assembly (GAMA) : stellar mass functions by Hubble type [PDF]
, 2014 This work was supported by the Austrian Science Foundation FWF under grant P23946. AWG was supported under the Australian Research Council's funding scheme FT110100263.We present an estimate of the galaxy stellar mass function and its division by ...
Alpaslan, Mehmet +24 more
core +4 more sources
The Effects of Environment on the Evolution of the Galaxy Stellar Mass Function [PDF]
, 2018 We study the effects of galaxy environment on the evolution of the stellar mass function (SMF) over 0.2 < z < 2.0 using the FourStar Galaxy Evolution (ZFOURGE) Survey and NEWFIRM Medium-Band Survey (NMBS) down to the stellar mass completeness limit, (9.5)
C. Papovich +10 more
semanticscholar +1 more source