Results 31 to 40 of about 18,267 (299)
The Stellar, Gas, and Dynamical Masses of Star-forming Galaxies at z ~ 2 [PDF]
, 2005 We present analysis of the near-infrared spectra of 114 rest-frame UV-selected star-forming galaxies at z ~ 2. By combining the Hα spectra with photometric measurements from observed 0.3-8 μm, we assess the relationships among kinematics, dynamical ...
Kurt L. Adelberger +12 more
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Planet gap opening across stellar masses
, 2020 Annular structures in protoplanetary discs, such as gaps and rings, are now ubiquitously found by high-resolution Atacama Large Millimetre Array observations.
Catriona A Sinclair +3 more
core +2 more sources
Radio observations of stellar mass loss [PDF]
Symposium - International Astronomical Union, 1979 A program to search for steady-state thermal emissions from stars has been in progress for several years in Canada (Purton 1976). In this program we have specifically excluded flaring objects (such as β Lyr or HR1099) where non-thermal emission is probably responsible.
Sun Kwok, C. R. Purton
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, 2015 This work is supported by the European Research Council/European Community under the FP7 through Starting Grant agreement number 239953. N.C.S. was supported by FCT through the Investigador FCT contract reference IF/00169/2012 and POPH/FSE (EC) by FEDER ...
Mortier, Annelies +18 more
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On the Stellar Masses of Giant Clumps in Distant Star-forming Galaxies [PDF]
, 2017 We analyze stellar masses of clumps drawn from a compilation of star-forming galaxies at 1.1 < z < 3.6. Comparing clumps selected in different ways, and in lensed or blank field galaxies, we examine the effects of spatial resolution and sensitivity on ...
Schaerer, Daniel +4 more
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The massive end of the stellar mass function [PDF]
Monthly Notices of the Royal Astronomical Society, 2015 11 pages, 8 figures, Accepted to ...
D'Souza, R., Vegetti, S., Kauffmann, G.
openaire +3 more sources
The Impact of Environment on the Stellar Mass–Halo Mass Relation [PDF]
The Astrophysical Journal, 2018 Abstract A large variance exists in the amplitude of the stellar mass–halo mass (SMHM) relation for group- and cluster-size halos. Using a sample of 254 clusters, we show that the magnitude gap between the brightest central galaxy (BCG) and its second or fourth brightest neighbor accounts for a significant portion of this variance.
Jesse B. Golden-Marx +1 more
openaire +2 more sources
Critical Rates of Stellar Mass Loss [PDF]
Symposium - International Astronomical Union, 1979 Many of the effects of mass loss on OB stars have now been explored. Mass loss will cause a star to be overluminous for its mass (though less luminous than a star of its original mass) and, for moderate mass-loss rates, the luminosity decreases at the same rate as the mass contained in the convective core decreases causing the main sequence lifetime to
D. S. P. Dearborn, J. B. Blake
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Pediatric Blood &Cancer, EarlyView.ABSTRACT Background Wilms tumor (WT) treatment imposes a significant time burden on patients and their families. Time toxicity is a patient‐centered metric that quantifies the burden of healthcare interaction. We sought to define time toxicity in the first year after diagnosis of WT and hypothesized that it would increase as tumor stage and treatment ...
Caleb Q. Ashbrook +6 more
wiley +1 more source
Photometric Stellar Parameters for Asteroseismology and Galactic Studies
, 2014 Asteroseismology has the capability of delivering stellar properties which would otherwise be inaccessible, such as radii, masses and thus ages of stars.
Casagrande, Luca, Luca Casagrande
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