Results 131 to 140 of about 5,163,973 (225)
The Hamburg/SAO Survey for Emission–Line Galaxies
We present first results of the Hamburg/SAO Survey for Emission-Line Galaxies (HSS therein, SAO – Special Astrophysical Observatory, Russia) which is based on the digitized objective-prism photoplates database of the Hamburg Quasar Survey (HQS). The main
D. Engels +9 more
core +1 more source
We study outflows in 130 galaxies with −22
Yi Xu +7 more
doaj +1 more source
An optical and infrared analysis of blue compact dwarf galaxies [PDF]
An understanding of Blue Compact Dwarf galaxies (BCDs) and the processes occurring within their chemically un-evolved environments is fundamental in our understanding of the early universe.
James, B.L.
core
The Hobby–Eberly Dark Energy Experiment (HETDEX) is an untargeted ∼540 deg ^2 spectroscopic survey of Ly α emission in the 1.9
Erin Mentuch Cooper +22 more
doaj +1 more source
Extremely Metal-poor Galaxies in DESI DR1: Connections to Galaxies in the Early Universe
Extremely metal-poor galaxies (XMPGs), defined as having metallicities below 10% of the solar value, are considered possible local analogs to primordial systems and offer a unique window into early galaxy evolution.
Jipeng Sui +45 more
doaj +1 more source
Thermal emission from H II galaxies: discovering the youngest systems [PDF]
We studied the radio properties of very young massive regions of star formation in HII galaxies, with the aim of detecting episodes of recent star formation in an early phase of evolution where the first supernovae start to appear. Our sample consists of
ELENA KIRILOVSKY TERLEVICH +2 more
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
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
Star formation powers optical line emission from the CGM. [PDF]
Zhang H +11 more
europepmc +1 more source
Stellar feedback drives the baryon deficiency in low-mass galaxies. [PDF]
Yu H +10 more
europepmc +1 more source

