Results 101 to 110 of about 1,176,456 (219)

Regarding the Detection of Interstellar C4 and C5 Molecules

open access: yesThe Astrophysical Journal
Analysis of very high signal-to-noise ratio (S/N) spectra of reddened stars allowed us to determine an upper limit (UL) of the column density N (C _4 ).
G. A. Galazutdinov   +2 more
doaj   +1 more source

Photoabsorption and photodissociation of molecules important in the interstellar medium [PDF]

open access: yes, 1985
The photoabsorption and photodissociation cross sections of several interstellar molecules and radicals in the 105 to 210 nm region were measured. The research results accomplished are briefly described.
Lee, L. C.
core  

An Ultraviolet Study of CO Chemistry in the Magellanic Clouds

open access: yesThe Astronomical Journal
How does molecular cloud chemistry change with metallicity? In this work, we study the relation between molecular hydrogen (H _2 ) and carbon monoxide (CO) at 1/2 and 1/5 solar metallicity using ultraviolet absorption spectroscopy obtained as part of the
Kirill Tchernyshyov   +2 more
doaj   +1 more source

Spectroscopy of cosmological molecules

open access: yes, 2023
The molecules in the interstellar medium are composed of atoms formed in supernovae. By studying the spectra of these molecules, we can better understand supernovae and the interstellar medium. This can be done in spectrometers on Earth.
Welch, Amy
core   +2 more sources

The Infrared Complex Refractive Index and Band Strengths of Coronene Thin Films

open access: yesThe Astrophysical Journal
Polycyclic aromatic hydrocarbon (PAH) molecules have long been theorized to be present in a multitude of interstellar environments. The radio-frequency detections of specific cyanosubstituted PAH molecules in the Taurus Molecular Cloud have provided new ...
J. E. Roser, L. Jovanović, A. Ricca
doaj   +1 more source

The relation between interstellar OH and other simple molecules

open access: yes, 2009
We discuss the close relation between the column densities of interstellar OH and CH molecules. Our results are obtained on the basis of 10 new sightlines.
Y. Beletsky   +3 more
core   +1 more source

The ALMA-QUARKS Survey: Properties of Hot Molecular Fragments in the Massive Protocluster IRAS 17233–3606

open access: yesThe Astrophysical Journal
To investigate the physical mechanisms of fragmentation within the hot molecular core of the massive protocluster IRAS 17233-3606 (G351.78-0.54), we carried out a detailed analysis of continuum and lines using the Atacama Large Millimeter/submillimeter ...
Li Chen   +31 more
doaj   +1 more source

Photoabsorption and photodissociation of molecules important in the interstellar medium [PDF]

open access: yes, 1986
In the period from May 15, 1985 to May 14, 1986, the photoabsorption and photodissociation cross sections of the interstellar radical of SO and the interstellar molecules of HCl, H2CO, and CH3CN were measured and the results were reported in scientific ...
Lee, L. C.
core  

Formation of All Three C2H4O Isomers—Ethylene Oxide (c-C2H4O), Acetaldehyde (CH3CHO), and Vinyl Alcohol (CH2CHOH)—in Ethanol-containing Interstellar Analog Ices

open access: yesThe Astrophysical Journal
Oxygen-containing complex organic molecules are key precursors to biorelevant compounds fundamental for the origins of life. However, the untangling of their interstellar formation mechanisms has just scratched the surface, especially for oxygen ...
Jia Wang   +3 more
doaj   +1 more source

Photoabsorption and photodissociation of molecules important in the interstellar medium [PDF]

open access: yes, 1987
A windowless apparatus was constructed and used to measure the photoabsorption and fluorescence cross sections of molecules in the extreme ultraviolet region.
Lee, Long C., Suto, Masako
core  

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