Results 111 to 120 of about 5,095,486 (206)
A Census from JWST of Extreme Emission-line Galaxies Spanning the Epoch of Reionization in CEERS
We present a sample of 1165 extreme emission-line galaxies (EELGs) at 4 < z < 9 selected using James Webb Space Telescope (JWST) NIRCam photometry in the Cosmic Evolution Early Release Science (CEERS) program.
Kelcey Davis +32 more
doaj +1 more source
Estimating the Sonic Mach Number in the Interstellar Medium with Convolutional Neural Networks
Understanding the role of turbulence in shaping the interstellar medium (ISM) is crucial for studying star formation, molecular cloud evolution, and cosmic-ray propagation.
Tyler Schmaltz, Yue Hu, Alex Lazarian
doaj +1 more source
Observations of O VI Emission from the Diffuse Interstellar Medium
International audienceWe report the first Far-Ultraviolet Spectroscopic Explorer measurements of diffuse O VI (λλ1032, 1038) emission from the general diffuse interstellar medium outside of supernova remnants or superbubbles.
Siegmund, O. H. W. +24 more
core +1 more source
Detailed Study of Stars and Gas in a z = 8.3 Massive Merger with Extreme Dust Conditions
We present galaxy MACS0416-Y1 at z _spec = 8.312 as observed by the CAnadian NIRISS Unbiased Cluster Survey. MACS0416-Y1 has been shown to have extreme dust properties; thus, we study the physical properties and star formation histories of its resolved ...
Anishya Harshan +17 more
doaj +1 more source
Gamma ray lines from interstellar grains [PDF]
The existence of very narrow (FWHM or approximately = 5 KeV) gamma ray line emission from interstellar grains is pointed out. The prime candidate for detection is the line at 6.129 Mev from O-16, but other very narrow lines could also be detected at 0 ...
Ramaty, R., Lingenfelter, R. E.
core
The Galactic Center Lobe as an H ii Region
The Galactic center lobe (GCL) is an object ∼1° across that is located north of the Galactic center. In the mid-infrared (MIR) the GCL appears as two 8.0 μ m filaments between which there is strong 24 μ m and radio continuum emission.
L. D. Anderson +7 more
doaj +1 more source
We present a catalog of 32,162 ^12 CO molecular clouds that covers the northern outer Galactic plane ( l = [15°, 165°] and l = [195°, 230°], and b = [−5.°25, +5.°25]).
Yan Sun +8 more
doaj +1 more source
Intensity mapping—the large-scale mapping of selected spectral lines without resolving individual sources—is quickly emerging as an efficient way to conduct large cosmological surveys. Multiple surveys covering a variety of lines (such as the hydrogen 21
Hannah Fronenberg, Adrian Liu
doaj +1 more source
The detection of circumstellar atomic hydrogen (H i ) via the 21 cm line remains a persistent challenge in planetary nebula (PN) studies, primarily due to contamination from ubiquitous interstellar H i 21 cm emission. In this paper, we report the results
Xu-Jia Ouyang +6 more
doaj +1 more source
Line-Leaking Models for Interstellar Molecular Emission and Absorption--I THE ANOMALOUS ABSORPTION AND EMISSION BY FORMALDEHYDE [PDF]
A. Margaret, D. ter Haar
openaire +1 more source

