Results 41 to 50 of about 17,065,072 (359)
Suppression of phase transitions and glass phase signatures in mixed cation halide perovskites
Nature Communications, 2020 Understanding the underlying physics and improving the performance of mixed lead halide perovskite materials remains a challenge. Here, the authors present experimental and theoretical study of structural phases, phase transitions, and dipolar dynamics ...
Mantas Simenas +14 more
doaj +1 more source
The Astrophysical Journal, 2023 We study the mass–size relation of quiescent galaxies across various environments, with a particular focus on its environmental dependence at the low-mass part of $\mathrm{log}({M}_{\mathrm{star}}/{M}_{\odot })\lesssim 10.0$ .
Yongmin Yoon, Jae-Woo Kim, Jongwan Ko
doaj +1 more source
Low-Mass Versus High-Mass Star Formation [PDF]
Symposium - International Astronomical Union, 1997 Structures like the clumps identified in the CO maps of the Rosette Molecular Cloud and the dense cores such as those in B5, a cluster of cores and young low-mass stars, are key to considerations of star formation. Whether star formation is a self-inducing process or one that causes itself to turn off depends greatly on whether the responses of the ...
T. W. Hartquist, J. E. Dyson
openaire +1 more source
The ALFALFA H I mass function: a dichotomy in the low-mass slope and a locally suppressed `knee' mass [PDF]
, 2018 The authors acknowledge the work of the entire ALFALFA collaboration in observing, flagging, and extracting the catalogue of galaxies that this paper makes use of.
Michael G. Jones +3 more
semanticscholar +1 more source
Scientific Reports, 2021 Previous studies on the association between thyroid function and body composition are conflicting and showed strong differences across age groups. Our aim was to clarify age-specific associations of serum thyroid-stimulating hormone (TSH) levels with ...
Till Ittermann +7 more
doaj +1 more source
On the Role of Dissolved Gases in the Atmosphere Retention of Low-mass Low-density Planets [PDF]
, 2018 Low-mass low-density planets discovered by Kepler in the super-Earth mass regime typically have large radii for their inferred masses, implying the presence of H2–He atmospheres. These planets are vulnerable to atmospheric mass loss due to heating by the
Yayaati Chachan, D. Stevenson
semanticscholar +1 more source
THE MASS-RADIUS(-ROTATION?) RELATION FOR LOW-MASS STARS [PDF]
The Astrophysical Journal, 2011 Accepted to ApJ; 21 pages, 10 figures, 8 tables in emulateapj format.
Kraus, Adam L. +4 more
openaire +3 more sources
Unstable low-mass planetary systems as drivers of white dwarf pollution [PDF]
, 2017 At least 25 percent of white dwarfs show atmospheric pollution by metals, sometimes accompanied by detectable circumstellar dust/gas discs or (in the case of WD 1145+017) transiting disintegrating asteroids.
A. Mustill +4 more
semanticscholar +1 more source
A Discontinuity in the Low‐Mass Initial Mass Function [PDF]
The Astrophysical Journal, 2007 The origin of brown dwarfs (BDs) is still an unsolved mystery. While the standard model describes the formation of BDs and stars in a similar way recent data on the multiplicity properties of stars and BDs show them to have different binary distribution functions.
Thies, Ingo, Kroupa, Pavel
openaire +2 more sources
Low-mass dark matter search with CDMSlite [PDF]
, 2017 Author(s): Agnese, R; Anderson, AJ; Aralis, T; Aramaki, T; Arnquist, IJ; Baker, W; Balakishiyeva, D; Barker, D; Basu Thakur, R; Bauer, DA; Binder, T; Bowles, MA; Brink, PL; Bunker, R; Cabrera, B; Caldwell, DO; Calkins, R; Cartaro, C; Cerdeno, DG; Chang ...
R. Agnese +106 more
semanticscholar +1 more source