Results 151 to 160 of about 210,358 (255)

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

A three-dimensional reconstruction of the interstellar magnetic field toward a star-forming region

open access: yesAstronomy & Astrophysics
Context. The polarized thermal emission from interstellar dust offers a valuable tool for probing both the dust and the magnetic field in the interstellar medium (ISM). However, existing observations only yield the total amount of dust emission along the
Ferrière K.   +2 more
doaj   +1 more source

Evidence for a multiphase, inhomogeneous interstellar medium in damped Ly alpha systems [PDF]

open access: yes
The large optical depth in absorption of the Ly-alpha line in damped Ly-alpha systems implies that the emission line produced by H2 regions is very broad, since the number of diffusions is very large.
Valls-Gabaud, David
core   +1 more source

Far infra-red emission lines in high redshift quasars

open access: yes, 2012
We present Plateau de Bure Interferometer observations of far infra-red emission lines in BRI 0952-0115, a lensed quasar at z=4.4 powered by a super-massive black hole (M_BH=2x10^9 M_sun).
Gallerani, Simona
core  

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

The role of radiative torques in the molecular cloud core L43

open access: yesAstronomy & Astrophysics
Context. Polarized emission from interstellar dust grains is commonly used to infer information about the underlying magnetic field from the diffuse interstellar medium to molecular cloud cores.
Scheiter M. L., Wolf S.
doaj   +1 more source

ELFO: A Python Package for Emission Line Fitting Optimization in Integral Field Spectroscopy Data

open access: yesThe Astronomical Journal
Integral field spectroscopy (IFS) provides spatially resolved spectra, enabling detailed studies that address the physical and kinematic properties of the interstellar medium.
Hui Guo   +6 more
doaj   +1 more source

Radio Jet Feedback on the Inner Disk of Virgo Spiral Galaxy Messier 58

open access: yesThe Astrophysical Journal
Spitzer spectral maps reveal a disk of highly luminous, warm (>150 K) H _2 in the center of the massive spiral galaxy Messier 58, which hosts a radio-loud active galactic nucleus (AGN). The inner 2.6 kpc of the galaxy appears to be overrun by shocks from
Patrick M. Ogle   +11 more
doaj   +1 more source

Investigating the Interstellar Medium Conditions of Star Formation in High Redshift Galaxies by studying Dust Emission and Emission lines

open access: yes, 2015
This thesis presents the search for the \cii 158 $\mu$m emission line, one of the brightest far-infrared (FIR) emission lines, in a selection of $z>6$ (the Universe was less than 1 Gyr old) galaxies. These galaxies have been observed with CARMA and PdBI millimeter interferometers and no \cii nor continuum emission is detected.
openaire   +2 more sources

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