Results 161 to 170 of about 266,062 (301)
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
Relativistic jets in narrow-line Seyfert 1 galaxies. New discoveries and open questions
Before the launch of the Fermi satellite only two classes of AGNs were known to produce relativistic jets and thus emit up to the γ-ray energy range: blazars and radio galaxies, both hosted in giant elliptical galaxies.
D’Ammando F. +4 more
doaj +1 more source
We present measurements of 5-25 {\mu}m emission features of brightest cluster galaxies (BCGs) with strong optical emission lines in a sample of 9 cool-core clusters of galaxies observed with the Infrared Spectrograph on board the Spitzer Space Telescope.
Aaron Hoffer +78 more
core +1 more source
Asymmetric emission of the [OIII]λ5007 profile in narrow-line Seyfert 1 galaxies [PDF]
E. O. Schmidt +4 more
openalex +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 at z = 6.5
2 pages, no figures, to be published in "Multiwavelength mapping of galaxy formation and evolution", proceedings of a conference held in Venice, October 13-16 2003, one typographic error ...
Kurk, Jaron +4 more
openaire +2 more sources
The formation and evolution of galaxies are intricately linked to the baryon cycle, which fuels star formation while shaping chemical abundances within galaxies.
Vicente Estrada-Carpenter +18 more
doaj +1 more source
Morphology and Evolution of Emission‐Line Galaxies in the Hubble Ultra Deep Field [PDF]
N. Pirzkal +10 more
openalex +1 more source
A tentative ∼1000 km s−1 offset between the [CII] 158 m and Lyα line emission in a star-forming galaxy at z = 7.2 [PDF]
R. Baier-Soto +6 more
openalex +1 more source
FUSEObservation of the Narrow‐Line Seyfert 1 Galaxy RE 1034+39: Dependence of Broad Emission Line Strengths on the Shape of the Photoionizing Spectrum [PDF]
D. Casebeer, Karen M. Leighly, E. Baron
openalex +1 more source

