Results 121 to 130 of about 11,157 (237)
Active galactic nuclei (AGNs), star formation (SF), and galaxy interactions can drive turbulence in the gas of the interstellar medium (ISM), which, in turn, plays a role in SF taking place within galaxies.
Riffel Rogemar A. +33 more
doaj +1 more source
Supplementary material to DESI's publication "DESI Emission Line Galaxies: Unveiling the Diversity of [OII] Profiles and its Links to Star Formation and Morphology" to comply with the data management plan.Ting-Wen Lan et al.Peer ...
Lan, Ting-Wen +4 more
core +1 more source
The clustering of galaxies in hierarchical galaxy formation models [PDF]
Galaxy clustering encodes information about the values of cosmological parameters and also about the physical processes behind galaxy formation and evolution. The GALFORM semi-analytical model is the theoretical approach we used to model galaxy formation.
KIM, HAN,SIK, Kim, Han Sik
core
A search for double-peaked narrow emission line galaxies and AGNs in the LAMOST DR1
International audienceThe Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) has released more than two million spectra, which provide the opportunity to search for double-peaked narrow emission line (NEL) galaxies and active galactic ...
Shen, Shi-Yin +17 more
core +1 more source
The Hamburg/SAO survey for emission-line galaxies
We present the sixth list with results of the Hamburg/SAO Survey for Emission-Line Galaxies. The final list resulted from follow-up spectroscopy conducted with the 4.5 m MMT telescope in 1996, and with 2.2 m CAHA and 6 m SAO telescopes in 2000 to 2003 ...
D. Engels +29 more
core +1 more source
Context. The comoving cosmic star formation rate density peaks at z ∼ 2–3, with dusty star-forming galaxies being significant contributors to this peak.
Kade K. +6 more
doaj +1 more source
Emission line galaxies in a narrow strip toward Perseus
Many studies have suggested that emission line galaxies (ELG's) have spatial distributions that differ from non-emission line galaxies. The ELG's tend to avoid rich clusters and may sometimes reside within voids.
Ellman, Nancy E.
core
Emission line imaging of 3CR quasars and radio galaxies
Optical emission line images and spectra of sixteen 3CR powerful radio galaxies and quasars are presented. Extended line emission is detected in both radio galaxies and quasars.
Barthel, PD, Hes, R, Fosbury, RAE
core +1 more source
Emission-line Diagnostics at z > 4: [O iii]λ4364/Hγ versus [Ne iii]λ3870/[O ii]λ3730
We use JWST Near-Infrared Spectrograph observations from the Cosmic Evolution Early Release survey, GLASS-JWST ERS (GLASS), and JWST Advanced Deep Extragalactic Survey to measure rest-frame optical emission-line ratios of 89 galaxies at z > 4.
Bren E. Backhaus +20 more
doaj +1 more source
The JWST EXCELS Survey: Insights into the Nature of Quenching at Cosmic Noon
We study 24 massive quiescent galaxies with $\mathrm{log}{{M}}_{* }/{{M}}_{\odot }\gt 10$ at 1
Maya Skarbinski +21 more
doaj +1 more source

