Results 11 to 20 of about 793,175 (240)

Benchmark Studies on the Isomerization Enthalpies for Interstellar Molecular Species

open access: yesJournal of Nigerian Society of Physical Sciences, 2023
With the well-established correlation between the relative stabilities of isomers and their interstellar abundances coupled with the prevalence of isomeric species among the interstellar molecular species, isomerization remains a plausible formation ...
Emmanuel Etim (PhD)
doaj   +1 more source

Ionize Hard: Interstellar PO+ Detection

open access: yesFrontiers in Astronomy and Space Sciences, 2022
We report the first detection of the phosphorus monoxide ion (PO+) in the interstellar medium. Our unbiased and very sensitive spectral survey toward the G+0.693–0.027 molecular cloud covers four different rotational transitions of this molecule, two of ...
Víctor M. Rivilla   +17 more
doaj   +1 more source

Abundance Ratios of OH/CO and HCO+/CO as Probes of the Cosmic-Ray Ionization Rate in Diffuse Clouds

open access: yesThe Astrophysical Journal, 2023
The cosmic-ray ionization rate (CRIR, ζ _2 ) is one of the key parameters controlling the formation and destruction of various molecules in molecular clouds. However, the current most commonly used CRIR tracers, such as ${{\rm{H}}}_{3}^{+}$ , OH ^+ , and
Gan Luo   +8 more
doaj   +1 more source

Calibrating Interstellar Abundances Using Supernova Remnant Radiative Shocks [PDF]

open access: yesAstronomical Journal, 2018
Using integral field data we extract the optical spectra of shocked interstellar clouds in Kepler’s supernova remnant located in the inner regions of our Galaxy, as well as in the Large Magellanic Cloud, the Small Magellanic Cloud, NGC 6822, and IC 1613.
M. Dopita   +6 more
semanticscholar   +1 more source

Quantum mechanical modeling of interstellar molecules on cosmic dusts: H2O, NH3, and CO2

open access: yesFrontiers in Chemistry, 2022
Since the first detection of CH molecule in interstellar medium (ISM), more than 270 molecules have been identified in various astronomical sources in ISM.
Fangfang Li   +9 more
doaj   +1 more source

First Glycine Isomer Detected in the Interstellar Medium: Glycolamide (NH2C(O)CH2OH) [PDF]

open access: yesAstrophysical Journal Letters, 2023
We report the first detection in the interstellar medium (ISM) of a C2H5O2N isomer: syn-glycolamide (NH2C(O)CH2OH). The exquisite sensitivity at sub-mK levels of an ultradeep spectral survey carried out with the Yebes 40 m and IRAM 30 m telescopes toward
V. Rivilla   +15 more
semanticscholar   +1 more source

The Distribution of Metallicities in the Local Galactic Interstellar Medium

open access: yesThe Astrophysical Journal, 2023
In this investigation, we present an analysis of the metallicity distribution that pertains to neutral gas in the local Galactic interstellar medium (ISM).
Adam M. Ritchey   +5 more
doaj   +1 more source

Survey of CH3NH2 and its Formation Process

open access: yesThe Astrophysical Journal, 2023
We present the observational results of a precursor of glycine, methylamine (CH _3 NH _2 ), together with methanol (CH _3 OH) and methanimine (CH _2 NH) for the high-mass star-forming regions NGC 6334I, G10.47+0.03, G31.41+0.3, and W51 e1/e2 using the ...
Taiki Suzuki   +9 more
doaj   +1 more source

A Reexamination of Phosphorus and Chlorine Depletions in the Diffuse Interstellar Medium

open access: yesThe Astrophysical Journal, 2023
We present a comprehensive examination of interstellar P and Cl abundances based on an analysis of archival spectra acquired with the Space Telescope Imaging Spectrograph of the Hubble Space Telescope and the Far Ultraviolet Spectroscopic Explorer ...
Adam M. Ritchey   +3 more
doaj   +1 more source

Boron abundances in diffuse interstellar clouds [PDF]

open access: yesProceedings of the International Astronomical Union, 2009
AbstractWe present a comprehensive survey of B abundances in diffuse interstellar clouds from HST/STIS observations along 56 Galactic sight lines. Our sample is the result of a complete search of archival STIS data for the B II λ1362 resonance line, with each detection confirmed by the presence of absorption from other dominant ions at the same ...
Ritchey, A. M.   +3 more
openaire   +2 more sources

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