Results 11 to 20 of about 111,392 (348)

Irradiated brown dwarfs

open access: yes, 2014
5 pages, 2 figures.
Casewell, S. L.   +5 more
openaire   +3 more sources

Search for brown-dwarf companions of stars [PDF]

open access: green, 2010
The discovery of 9 new brown-dwarf candidates orbiting stars in the CORALIE and HARPS radial-velocity surveys is reported. New CORALIE radial velocities yielding accurate orbits of 6 previously-known hosts of potential brown-dwarf companions are ...
J. Sahlmann   +9 more
openalex   +4 more sources

The brown dwarf desert as a consequence of orbital migration [PDF]

open access: yes, 2001
We show that the dearth of brown dwarfs in short-period orbits around Solar-mass stars - the brown dwarf desert - can be understood as a consequence of inward migration within an evolving protoplanetary disc.
Armitage   +37 more
core   +3 more sources

The Galactic disk mass-budget : II. Brown dwarf mass-function and density [PDF]

open access: yes, 2001
In this paper, we extend the calculations conducted previously in the stellar regime to determine the brown dwarf IMF in the Galactic disk. We perform Monte Carlo calculations taking into account the brown dwarf formation rate, spatial distribution and ...
Chabrier G.   +6 more
core   +2 more sources

Disk or Companion: Characterizing Excess Infrared Flux in Seven White Dwarf Systems with Near-infrared Spectroscopy

open access: yesThe Astronomical Journal, 2023
Excess infrared flux from white dwarf stars is likely to arise from a dusty debris disk or a cool companion. In this work, we present near-infrared spectroscopic observations with Keck/MOSFIRE, Gemini/GNIRS, and Gemini/Flamingos-2 of seven white dwarfs ...
Dylan Owens   +9 more
doaj   +1 more source

SMA observations of the proto brown dwarf candidate SSTB213 J041757 [PDF]

open access: yes, 2014
Context. The previously identified source SSTB213 J041757 is a proto brown dwarf candidate in Taurus, which has two possible components A and B. It was found that component B is probably a class 0/I proto brown dwarf associated with an extended envelope.
C. -f. Lee   +4 more
core   +1 more source

The Oceanus Moving Group: A New 500 Myr Old Host for the Nearest Brown Dwarf

open access: yesThe Astrophysical Journal, 2023
We report the discovery of the Oceanus moving group, a ≈500 Myr old group with 50 members and candidate members at distances 2–50 pc from the Sun, using an unsupervised clustering analysis of nearby stars with Gaia DR3 data.
Jonathan Gagné   +7 more
doaj   +1 more source

Possible nuclear fusion of deuteron in the cores of Earth, Jupiter, Saturn, and brown dwarfs

open access: yesAIP Advances, 2020
Many brown dwarfs have recently been discovered as sub-stellar objects in which deuteron thermonuclear fusion is taking place. Although Jupiter and Saturn emit nearly twice as much heat as they absorb from the Sun, their internal heat-generation ...
Mikio Fukuhara
doaj   +1 more source

Устойчивость ячменя озимого к основным болезням в условиях западной лесостепи Украины

open access: yesAgricultural Science, 2021
The results of three years of research on the influence of meteorological factors on the degree of damage to winter barley varieties by basic diseases are presented.
Галина БИЛОВУС
doaj   +1 more source

Astrometric Accelerations as Dynamical Beacons: Discovery and Characterization of HIP 21152 B, the First T-dwarf Companion in the Hyades

open access: yesThe Astronomical Journal, 2023
Benchmark brown dwarf companions with well-determined ages and model-independent masses are powerful tools to test substellar evolutionary models and probe the formation of giant planets and brown dwarfs.
Kyle Franson   +30 more
doaj   +1 more source

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