Results 21 to 30 of about 149 (117)

Exploring the gaseous halos of z > 3 radio galaxies with UVES and JWST/NIRSpec

open access: yesAstronomy & Astrophysics
High-redshift radio galaxies are among the most massive galaxies in the Universe and sites of extreme active galactic nucleus feedback processes, powering energetic radio jets.
Ritter Jelena   +5 more
doaj   +1 more source

MUSE Analysis of Gas around Galaxies (MAGG)

open access: yesAstronomy & Astrophysics
We investigate the connection between strong, blended Lyα absorption systems (SBLAs) and ≈1000 Lyα-emitting galaxies (LAEs) at z ≳ 3 in 28 quasar fields from the MUSE Analysis of Gas around Galaxies (MAGG) survey. Selecting SBLAs as spectral regions with
Galbiati Marta   +4 more
doaj   +1 more source

Delayed Massive-star Mechanical Feedback at Low Metallicity

open access: yesThe Astrophysical Journal, 2023
The classical model of massive-star mechanical feedback is based on effects at solar metallicity ( Z _⊙ ), yet feedback parameters are very different at low metallicity.
Michelle C. Jecmen, M. S. Oey
doaj   +1 more source

BLUEPRINT: Blue-dominant Lyman-α emission as evidence of gas inflow in ultra-low-mass galaxies at z = 3

open access: yesAstronomy & Astrophysics
We report the detection of a clumpy, blue-dominated Lyman-α (Lyα) emission at z = 3.066 located in the heart of a cosmic web filament in the MUSE eXtremely Deep Field (MXDF).
Mukherjee Tamal   +6 more
doaj   +1 more source

GA-NIFS: AGN activity in a Lyα emitter within a triple-AGN system anchored by a passive galaxy at z = 3

open access: yesAstronomy & Astrophysics
Context. Massive quenched galaxies at z > 3 challenge models of early galaxy evolution, as their rapid formation and abrupt quenching require efficient feedback, which is often linked to active galactic nuclei (AGNs).
Perna Michele   +17 more
doaj   +1 more source

Using Lyα Absorption to Measure the Intensity and Variability of z ∼ 2.4 Ultraviolet Background Light

open access: yesThe Astrophysical Journal
We present measurements of z  ∼ 2.4 ultraviolet (UV) background light using Ly α absorption from galaxies at z  ∼ 2–3 in the Hobby–Eberly Telescope Dark Energy Experiment (HETDEX) database.
Laurel H. Weiss   +13 more
doaj   +1 more source

A Cosmic Archipelago of lensed metal-poor galaxies at z ∼ 6

open access: yesAstronomy & Astrophysics
The Cosmic Archipelago is an ensemble of galaxies, strongly lensed by the Hubble Frontier Fields cluster MACS J0416, displaying some of the most extreme physical properties known at z ~ 6.14.
Bolamperti A.   +23 more
doaj   +1 more source

Extreme equivalent-width-selected low-mass starbursts at z = 4 − 9: Insights into their role in cosmic reionization

open access: yesAstronomy & Astrophysics
We investigate the properties of extreme emission line galaxies (EELGs) at z = 4 − 9 and their role in reionization. Compact, low-mass galaxies with intense optical emission lines are linked to elevated specific star formation rates (sSFRs) and recent ...
Llerena M.   +24 more
doaj   +1 more source

The Lyα Reference Sample. XIV. Lyα Imaging of 45 Low-redshift Star-forming Galaxies and Inferences on Global Emission

open access: yesThe Astrophysical Journal Supplement Series, 2023
We present Ly α imaging of 45 low-redshift star-forming galaxies observed with the Hubble Space Telescope. The galaxies have been selected to have moderate to high star formation rates (SFRs) using far-ultraviolet (FUV) luminosity and H α equivalent ...
Jens Melinder   +20 more
doaj   +1 more source

MAMMOTH-Subaru. IV. Large Scale Structure and Clustering Analysis of Lyα Emitters and Lyα Blobs at z = 2.2–2.3

open access: yesThe Astrophysical Journal
We report the large scale structure and clustering analysis of Ly α emitters (LAEs) and Ly α blobs (LABs) at z  = 2.2–2.3. Using 3341 LAEs, 117 LABs, and 58 bright (Ly α luminosity L _Ly _α  > 10 ^43.4 erg s ^−1 ) LABs at z  = 2.2–2.3 selected with ...
Haibin Zhang   +12 more
doaj   +1 more source

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