The Lyman Continuum Escape Fraction of Emission Line-selected z ∼ 2.5 Galaxies Is Less Than 15% [PDF]
Recent work suggests that strong emission line, star-forming galaxies (SFGs) may be significant Lyman continuum leakers. We combine archival Hubble Space Telescope broadband ultraviolet and optical imaging (F275W and F606W, respectively) with emission ...
M. Rutkowski +11 more
semanticscholar +1 more source
ABSTRACT Planetary nebulae represent a late evolutionary phase of low‐ to intermediate‐mass stars. In this article, we present the serendipitous discovery of a previously unknown, faint potential Galactic planetary nebula (PN) in the constellation Camelopardalis, identified during a survey‐inspection, aiming at the detection of dwarf companions of the ...
W. E. Celnik +12 more
wiley +1 more source
We present near-infrared spectra with resolutions of lambda/dlambda~1200 in the emission lines of Pa-beta, [FeII] (1.2567um), Br-gamma, and H2 v=1-0S(1) of the nuclei and circumnuclear regions of the four Seyfert 2 galaxies Mk 1066, NGC 2110, NGC 4388 ...
B. T. Soifer +16 more
core +1 more source
THE NATURE OF EXTREME EMISSION LINE GALAXIES AT z = 1–2: KINEMATICS AND METALLICITIES FROM NEAR-INFRARED SPECTROSCOPY [PDF]
We present near-infrared spectroscopy of a sample of 22 Extreme Emission Line Galaxies at redshifts 1.3 < z < 2.3, confirming that these are low-mass (M⋆ = 108–109 M☉) galaxies undergoing intense starburst episodes (M⋆/SFR ∼ 10–100 Myr).
M. Maseda +23 more
semanticscholar +1 more source
Extended Emission Lines in Radio Galaxies [PDF]
In whatever physical state the gas is found, observations of the interstellar medium in elliptical galaxies are of considerable interest. This is particularly true in the case of radio galaxies where we believe that the gas is an indespensable part of the cause of nuclear activity and plays a role in the origin and the evolution of the radio galaxy ...
openaire +1 more source
Gone with the heat: a fundamental constraint on the imaging of dust and molecular gas in the early Universe [PDF]
Images of dust continuum and carbon monoxide (CO) line emission are powerful tools for deducing structural characteristics of galaxies, such as disc sizes, H2 gas velocity fields and enclosed H2 and dynamical masses. We report on a fundamental constraint
Zhi-Yu Zhang +5 more
doaj +1 more source
Synthetic nebular emission from massive galaxies - I: origin of the cosmic evolution of optical emission-line ratios [PDF]
Galaxies occupy different regions of the [OIII]$\lambda5007$/H$\beta$-versus-[NII]$\lambda6584$/H$\alpha$ emission-line ratio diagram in the distant and local Universe.
M. Hirschmann +6 more
semanticscholar +1 more source
Survey on AI‐Enabled Computer Vision Technologies and Applications for Space Robotic Missions
ABSTRACT This survey provides a comprehensive overview of recent advancements and challenges in Artificial Intelligence (AI)‐enabled computer vision (CV) techniques for space robotic missions, spanning critical phases such as Entry, Descent, and Landing (EDL), orbital operations, and planetary surface exploration.
Maciej Quoos +6 more
wiley +1 more source
On the Nature of the Strong Emission-Line Galaxies in Cluster Cl 0024+1654: Are Some the Progenitors of Low Mass Spheroidals? [PDF]
We present new size, line ratio, and velocity width measurements for six strong emission-line galaxies in the galaxy cluster, Cl 0024+1654, at redshift z~0.4.
Babul A. +6 more
core +3 more sources
Extreme emission-line galaxies out to z$\sim$1 in zCOSMOS. I. Sample and characterization of global properties [PDF]
We present a thorough characterization of a large sample of 183 extreme emission-line galaxies (EELGs) at redshift 0 ...
R. Amor'in +38 more
semanticscholar +1 more source

