Results 111 to 120 of about 1,223,277 (388)
THE RELATION BETWEEN STAR FORMATION RATE AND STELLAR MASS FOR GALAXIES AT 3.5 ⩽ z ⩽ 6.5 IN CANDELS [PDF]
Distant star-forming galaxies show a correlation between their star formation rates (SFRs) and stellar masses, and this has deep implications for galaxy formation. Here, we present a study on the evolution of the slope and scatter of the SFR–stellar mass
B. Salmon +17 more
semanticscholar +1 more source
ABSTRACT Background B‐cell lymphoblastic lymphoma (B‐LBL) represents a rare variety of non‐Hodgkin lymphoma, with limited research on its biology, progression, and management. Methods A retrospective analysis was performed on the clinical characteristics of 256 patients aged ≤18 years who received treatment under the China Net Childhood Lymphoma (CNCL)‐
Zhijuan Liu +20 more
wiley +1 more source
The Supersonic Project: Early Star Formation with the Streaming Velocity
At high redshifts ( z ≳ 12), the relative velocity between baryons and dark matter (the so-called streaming velocity) significantly affects star formation in low-mass objects.
William Lake +9 more
doaj +1 more source
Star Formation Law at Sub-kpc Scale in the Elliptical Galaxy Centaurus A as Seen by ALMA
We present an extensive analysis of the relationship between star formation rate surface density (∑SFR) and molecular gas surface density (∑H2) at sub-kpc scale in the elliptical galaxy Centaurus A (also known as NGC 5128) at the distance 3.8 Mpc.
Jazeel H. Azeez +3 more
doaj +1 more source
An Extremely Compact, Low-mass Galaxy on its Way to Quiescence at z = 5.2
We report the discovery of a low-mass z = 5.200 ± 0.002 galaxy that is in the process of ceasing its star formation. The galaxy, MACS0417-z5BBG, is multiply imaged with magnification factors ∼40 by the galaxy cluster MACS J0417.5-1154, observed as part ...
Victoria Strait +17 more
doaj +1 more source
It is generally assumed that a large fraction of stars are initially born in clusters. However, a large fraction of these disrupt on short timescales and the stars end up belonging to the field. Understanding this process is of paramount importance if we
Annibali +53 more
core +4 more sources
Quenching or Bursting: Star Formation Acceleration--A New Methodology for Tracing Galaxy Evolution [PDF]
We introduce a new methodology for the direct extraction of galaxy physical parameters from multi-wavelength photometry and spectroscopy. We use semi-analytic models that describe galaxy evolution in the context of large scale cosmological simulation to ...
Darvish, Behnam +4 more
core +2 more sources
The density structure and star formation rate of non-isothermal polytropic turbulence [PDF]
The interstellar medium of galaxies is governed by supersonic turbulence, which likely controls the star formation rate (SFR) and the initial mass function (IMF).
C. Federrath, S. Banerjee
semanticscholar +1 more source
Star Formation Rate Determinations
12 pages, 4 figures; to appear in the Proceedings of the conference `Pathways through an Eclectic Universe', J.H. Knapen, T.J. Mahoney, and A.
openaire +3 more sources
Impact of star formation history on the measurement of star formation rates [PDF]
10 pages, 10 figures, 1 table.
Boquien, M., Buat, V., Perret, V.
openaire +3 more sources

