Results 111 to 120 of about 1,993,973 (222)
ELT requirements for future observation of the intergalactic medium
We summarise the science cases for an ELT that were presented in the parallel session on the intergalactic medium, and the open discussion that followed the formal presentations.
Theuns, Tom +3 more
core +1 more source
In dwarf galaxy models, outflows expel metal-enriched interstellar medium (ISM) into the circumgalactic medium (CGM) to reproduce their observed low metallicities, but measurements of dwarf CGM properties are scarce.
Sean D. Johnson +15 more
doaj +1 more source
Observations of intergalactic HI in groups of southern galaxies
We started a program for searching HI in the intergalactic medium and in the direction to two groups of galaxies: NGC 5128 and NGC 6300. The minimum detectable mass in each group will be 5.8 x 10⁷ and 5.2x10⁸ solar masses respectively.Asociación ...
Martin, M.C.
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Continuous solutions of cosmic-rays and waves in astrophysical environments. [PDF]
Irshad K +5 more
europepmc +1 more source
How galaxies drive reionization and what governs its geometry remain fundamental questions. We present JWST/NIRCam wide-field slitless spectroscopy (WFSS) observations toward two of the most Ly α -transmissive QSO sight lines near the end of reionization.
Yongda Zhu +8 more
doaj +1 more source
Neutrino communication, intergalactic transit, and Astrobiology. [PDF]
Shapshak P.
europepmc +1 more source
When Does the Intergalactic Medium Become Enriched?
We use cosmological hydrodynamic simulations including galactic feedback based on observations of local starbursts to find a self-consistent evolutionary model capable of fitting the observations of the intergalactic metallicity history as traced by C ...
K. Finlator, R. Davé, B.D. Oppenheimer
core +1 more source
The 2023 Flight of the Faint Intergalactic-medium Redshifted Emission Balloon
The second iteration of the Faint Intergalactic-medium Redshifted Emission Balloon (FIREBall-2) is a UV multiobject spectrograph designed to detect emission from the circumgalactic and circumquasar medium at low redshifts ( z < 1).
Drew M. Miles +36 more
doaj +1 more source
Lyman limit systems (LLSs) are dense hydrogen clouds with high enough H i column densities to absorb Lyman continuum photons emitted from distant quasars.
Jiawen Fan +3 more
doaj +1 more source
X-ray absorption by the intergalactic medium
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.Includes bibliographical references (p. 145-155).I have studied the intergalactic medium (IGM) located in galaxy clusters and groups via the so-called "X-ray Forest" the X-ray
Fang, Taotao, 1970-
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