Results 71 to 80 of about 210,358 (255)
Interstellar H^+_3: possible detection of the 1_(10)→1_(11) transition of H_2D^+ [PDF]
An interstellar line has been detected in emission at the expected submillimeter wavelength of the 1_(10)→1_(11) transition of H_(2)D^+, the deuterated version of the primary ion (H^(+)_(3)) in the favored ion-molecule reaction scheme for interstellar ...
Blake, Geoffrey A. +4 more
core
Searching for an Intermediate Mass Black Hole in the Blue Compact Dwarf galaxy MRK 996 [PDF]
The possibility is explored that accretion on an intermediate mass black hole contributes to the ionisation of the interstellar medium of the Compact Blue Dwarf galaxy MRK996.
A. Aloisi +55 more
core +3 more sources
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
COBE Observations of Interstellar Line Emission
7 pages of LaTeX with 5 included figures.
openaire +2 more sources
Abstract 10Be deposition in ice cores is widely used for solar reconstructions, but its interpretation is complicated by volcanic influences. Using the state‐of‐the‐art aerosol‐climate model ECHAM6.3‐HAM2.3‐SALSA2.0: 10Be, we assess the impacts of three major volcanic eruptions: Agung (1963), El Chichón (1982) and Pinatubo (1991). All eruptions enhance
Minjie Zheng +8 more
wiley +1 more source
The H2 Glow of a Quiescent Molecular Cloud Observed with JWST
We report JWST MIRI/MRS observations of the H _2 S (1) 17.04 μ m transition in two regions in the boundary of the Taurus molecular cloud. The two regions, denoted “Edge” (near the relatively sharp boundary of the ^13 CO J = 1 → 0 emission) and “Peak ...
Paul F. Goldsmith +8 more
doaj +1 more source
CII in the Interstellar Medium: Excitation by H2 Revisited
C$^+$ is a critical constituent of many regions of the interstellar medium, as it can be a major reservoir of carbon and, under a wide range of conditions, the dominant gas coolant.
Goldsmith, Paul F., Wiesenfeld, Laurent
core +3 more sources
The Effect of Turbulence on Nebular Emission Line Ratios [PDF]
Motivated by the observed differences in the nebular emission of nearby and high redshift galaxies, we carry out a set of direct numerical simulations of turbulent astrophysical media exposed to a UV background.
W. Gray, E. Scannapieco
semanticscholar +1 more source
Recent development of cryogenic ion‐trap‐based instrumentation has extended the scope of gas‐phase laser spectroscopy to a wide variety of nonvolatile ions, including carbocations and protonated hydrocarbons, organic dyes, host‐guest complexes, micro‐hydrated ions, hypervalent ions, metal clusters, and ionic intermediates formed in solution.
Satoru Muramatsu +2 more
wiley +1 more source
Spatially Resolved Comparison of SFRs from UV and Hα in GASP Gas-stripped Galaxies
Star formation rates (SFRs) in galaxies offer a view of various physical processes across them, and are measured using various tracers, such as H α and ultraviolet (UV).
Neven Tomičić +8 more
doaj +1 more source

