Results 11 to 20 of about 3,434,376 (288)
Extragalactic Constraints on the Initial Mass Function [PDF]
The local stellar mass density is observed to be significantly lower than the value obtained from integrating the cosmic star formation history (SFH), assuming that all the stars formed with a Salpeter initial mass function (IMF).
Adelman-McCarthy +24 more
core +6 more sources
Initial mass function of intermediate mass black hole seeds [PDF]
We study the Initial Mass Function (IMF) and host halo properties of Intermediate Mass Black Holes (IMBH, 10^{4-6} Msun) formed inside metal-free, UV illuminated atomic cooling haloes (virial temperature T_vir > 10^4 K) either via the direct collapse of ...
Ferrara, A. +3 more
core +7 more sources
Theories of the initial mass function [PDF]
We review the various theories which have been proposed along the years to explain the origin of the stellar initial mass function. We pay particular attention to four models, namely the competitive accretion and the theories based respectively on ...
André +14 more
core +5 more sources
Toward an initial mass function for giant planets [PDF]
The distribution of exoplanet masses is not primordial. After the initial stage of planet formation is complete, the gravitational interactions between planets can lead to the physical collision of two planets, or the ejection of one or more planets from
Carrera, Daniel +2 more
core +2 more sources
Constraining the Initial Mass Function via Stellar Transients
The stellar initial mass function (IMF) represents a fundamental quantity in astrophysics and cosmology describing the mass distribution of stars from low mass all the way up to massive and very massive stars. It is intimately linked to a wide variety of
Francesco Gabrielli +6 more
doaj +3 more sources
On the variation of the Initial Mass Function [PDF]
(shortened) In this contribution an average or Galactic-field IMF is defined, stressing that there is evidence for a change in the power-law index at only two masses: near 0.5 Msun and 0.08 Msun.
Kroupa, Pavel
core +4 more sources
Mapping the core mass function to the initial mass function [PDF]
13 pages, 15 figures, accepted by MNRAS on 17 April ...
Guszejnov, Dávid, Hopkins, Philip F.
openaire +3 more sources
THE HIGH-MASS STELLAR INITIAL MASS FUNCTION IN M31 CLUSTERS [PDF]
11 pages, 7 Figures, submitted to ApJ.
Daniel R. Weisz +18 more
openaire +2 more sources
Fragmentation and the initial mass function [PDF]
A central problem in the theory of star formation is to understand the spectrum of masses, or Initial Mass Function, with which stars are formed. The fundamental role of the IMF in galactic evolution has been described by Tinsley (1980), and an extensive review of evidence concerning the IMF and its possible variability has been presented by Scalo ...
openaire +1 more source
A two-step initial mass function: [PDF]
If stars originate in transient bound clusters of moderate size, these clusters will decay due to dynamic interactions in which a hard binary forms and ejects most or all the other stars. When the cluster members are chosen at random from a reasonable initial mass function (IMF), the resulting binary characteristics do not match current observations ...
R. H. Durisen +2 more
openaire +1 more source

