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

open access: yesThe Astrophysical Journal
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

open access: yesThe Astrophysical Journal
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

open access: yes, 2001
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

open access: yesThe Astrophysical Journal Letters
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]

open access: yes, 1976
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

open access: yesThe Astrophysical Journal
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

Molecular Clouds in the Outer Milky Way Disk: Sample, Integrated Properties, and Radial Trends with Galactocentric Radius

open access: yesThe Astrophysical Journal Supplement Series
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

Forecasts and Statistical Insights for Line Intensity Mapping Cross-correlations: A Case Study with 21 cm × [C ii]

open access: yesThe Astrophysical Journal
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

FAST Search for Circumstellar Atomic Hydrogen. III. Planetary Nebulae at Galactic Latitudes ∣b∣ ≥ 10°

open access: yesThe Astronomical Journal
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

Home - About - Disclaimer - Privacy