Results 121 to 130 of about 11,157 (237)

Impact of active galactic nuclei and nuclear star formation on the ISM turbulence of galaxies: Insights from JWST/MIRI spectroscopy

open access: yesAstronomy & Astrophysics
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

DESI Emission Line Galaxies: Unveiling the Diversity of [OII] Profiles and its Links to Star Formation and Morphology [Dataset]

open access: yes
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]

open access: yes, 2010
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

open access: yes, 2014
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

open access: yes, 2005
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

Resolving the molecular gas emission of the z ∼ 2.5–2.8 starburst galaxies SPT 0125-47 and SPT 2134-50

open access: yesAstronomy & Astrophysics
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

open access: yes, 1993
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

open access: yes, 1996
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

open access: yesThe Astrophysical Journal
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

open access: yesThe Astrophysical Journal
We study 24 massive quiescent galaxies with $\mathrm{log}{{M}}_{* }/{{M}}_{\odot }\gt 10$ at 1 
Maya Skarbinski   +21 more
doaj   +1 more source

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