Results 91 to 100 of about 210 (157)

MOSEL Survey: Spatially Offset Lyman-continuum Emission in a New Emitter at z = 3.088 Can Explain the Low Number Density of Observed LyC Leakers

open access: yesThe Astrophysical Journal
We present the discovery of a unique Lyman-continuum (LyC) emitter at z = 3.088. The LyC emission was detected using the Hubble Space Telescope WFC3/UVIS F336W filter, covering a rest-frame wavelength range of 760–900 Å. The peak signal-to-noise ratio of
Anshu Gupta   +11 more
doaj   +1 more source

Properties of Low-Redshift Damped Lyman Alpha Galaxies

open access: yes, 2001
8 pages, 6 figures, uses newpasp.sty. To appear in ASP Conference Series "Extragalactic Gas at Low Redshift", J. Mulchaey and J.
Nestor, Daniel B.   +5 more
openaire   +2 more sources

The Stellar Origin of “V-shaped” Spectral Energy Distributions in Lyα-emitting Little Red Dots Revealed by JWST/MIRI

open access: yesThe Astrophysical Journal
Understanding the nature of the high-redshift “V-shaped” little red dots (LRDs) recently uncovered by the James Webb Space Telescope (JWST) is crucial for constraining the early coevolution of galaxies and supermassive black holes (SMBHs).
Jian Ren   +10 more
doaj   +1 more source

Chasing Lyman alpha-emitting galaxies at z = 8.8

open access: yes, 2018
Submitted to A&A, comments are ...
Laursen, Peter   +4 more
openaire   +2 more sources

Disentangling the galactic and intergalactic components in 313 observed Lyman-alpha line profiles between redshift 0 and 5

open access: yesThe Open Journal of Astrophysics
Lyman-Alpha (Ly$\alpha$) photons emitted in star-forming galaxies undergo complex radiative transfer through the interstellar (ISM), circumgalactic (CGM), and intergalactic medium (IGM), imprinting characteristic signatures on their observed line ...
Siddhartha Gurung-López   +7 more
doaj   +1 more source

Lyman-alpha Cooling Emission from Galaxy Formation

open access: yes, 2010
Recent studies have shown that galaxies accrete most of their baryons via the cold mode, from streams with temperatures T~10^4-10^5 K. At these temperatures, the streams should radiate primarily in the Lya line and have therefore been proposed as a model to power the extended, high-redshift objects known as Lya blobs and other high-redshift Lya sources.
Faucher-Giguere, C. -A.   +4 more
openaire   +2 more sources

Deciphering Spatially Resolved Lyman-Alpha Profiles in Reionization Analogs: The Sunburst Arc at Cosmic Noon

open access: yesThe Open Journal of Astrophysics
The hydrogen Lyman-alpha (Ly$\alpha$) emission line, the brightest spectral feature of a photoionized gas, is considered an indirect tracer of the escape of Lyman continuum (LyC) photons, particularly when the intergalactic medium is too opaque for ...
Erik Solhaug   +9 more
doaj   +1 more source

Constraining Reionization with Lyman Alpha Emitting Galaxies

open access: yes, 2015
17 pages, 6 figures. Book chapter in "Understanding the Epoch of Cosmic Reionization: Challenges and Progress", Springer International Publishing, Ed.
openaire   +2 more sources

Lyman alpha Emission from High-Redshift Galaxies

open access: yes, 1995
uuencoded compressed postscript.
Pettini, Max   +3 more
openaire   +2 more sources

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