Results 321 to 330 of about 15,774,260 (349)

Adsorption of copper(II) in biochar-humic acid-water system. [PDF]

Sci Rep
Li Y, Zhao B, Shang T.
europepmc   +1 more source

Exploring the extremes: The cosmic laboratory. [PDF]

Innovation (Camb)
Huang Y, He S, Ge L, Li Z, Mao Y, Liu J.
europepmc   +1 more source

Radiative cooling induced coherent maser emission in relativistic plasmas. [PDF]

Sci Adv
Bilbao P, Silva T, Silva LO.
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Accelerated Free Energy Estimation in <i>Ab Initio</i> Path Integral Monte Carlo Simulations. [PDF]

J Phys Chem Lett
Svensson P, Kalkavouras F, Hernandez Acosta U, Moldabekov ZA, Tolias P, Vorberger J, Dornheim T.   +6 more
europepmc   +1 more source

Identification of a turnover in the initial mass function of a young stellar cluster down to 0.5 MJ

De Furio M, Meyer M, Greene T, Hodapp K, Johnstone D, Leisenring J, Rieke M, Robberto M, Roellig T, Cugno G, Fiorellino E, Manara C, Raileanu R, Terwisga Sv.   +13 more
europepmc   +1 more source

An Abrupt Change in the Disk Fraction of Free-Floating Planets at the Deuterium-Burning Ignition Limit

Rodrigues T, Bouy H, Raymond S, Martín E, Bertin E, Romero JO, Barrado D, Huélamo N, Tamura M, Roig NM, Galli P, Cuillandre J.   +11 more
europepmc   +1 more source

Primeval very low-mass stars and brown dwarfs – VI. Population properties of metal-poor degenerate brown dwarfs [PDF]

Monthly Notices of the Royal Astronomical Society, 2019
We presented 15 new T dwarfs that were selected from UKIRT Infrared Deep Sky Survey, Visible and Infrared Survey Telescope for Astronomy , and Wide-field Infrared Survey Explorer surveys, and confirmed with optical to near-infrared spectra obtained ...
Adam J Burgasser, M C Gálvez-Ortiz, N Lodieu   +2 more
exaly   +2 more sources

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Very Cool L-Dwarfs

Science, 2000
ASTRONOMY Dwarfs are low mass, very cool, main-sequence stars, and recent large-scale star surveys have identified a new spectral class, called the L-dwarfs. The low estimated masses of L-dwarfs suggest that most of these objects are brown dwarfs that are rich in hydrides rather than methane. McLean et al. have obtained high-resolution spectra of six L-
openaire   +1 more source

Dwarfing in the raspberry, Rubus idaeus L.

Euphytica, 1969
Six phenotypically distinct dwarfs of the raspberry (Rubus idaeus L.) are described; two of them are digenic, ‘sturdy dwarf’ being D 1d1d2d2or d 1d1d2d2and ‘crumpled dwarf’ d 3d3d4d4. Jennings' (1967) dwdw dwarf appears to be phenotypically and genotypically identical with the digenic ‘sturdy’.
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Ultracool dwarfs observed with the Spitzer infrared spectrograph – II. Emergence and sedimentation of silicate clouds in L dwarfs, and analysis of the full M5–T9 field dwarf spectroscopic sample

Monthly Notices of the Royal Astronomical Society, 2022
Genaro Suarez, Stanimir Metchev
exaly