Results 141 to 150 of about 1,388 (238)
A SEARCH FOR INTERSTELLAR CARBON-CHAIN ALCOHOL HC4OH IN STAR-FORMING REGION L1527 AND DARK CLOUD TMC-1 [PDF]
Mitsunori Araki +8 more
openalex +1 more source
The most abundant interstellar molecule, molecular hydrogen (H _2 ), is practically invisible in cold molecular clouds. Astronomers typically use carbon monoxide (CO) to trace the bulk distribution and mass of H _2 in our galaxy and many others.
Michael P. Busch
doaj +1 more source
H2cs Abundances And Ortho-to-para Ratios In Interstellar Clouds
The published version is located at http://adsabs.harvard.edu/full/1991A%26A...244..181MSeveral H2CS ortho and para transitions have been observed toward interstellar molecular clouds, including cold, dark clouds and star-forming regions. H2CS fractional
BREWER, MK, MINH, YC, Irvine, William M.
core
The Resolved Structure of a Low-metallicity Photodissociation Region
Photodissociation regions (PDRs) are key to understanding the feedback processes that shape interstellar matter in galaxies. One important type of PDR is the interface between H ii regions and molecular clouds, where far-ultraviolet radiation from ...
Ilyse Y. Clark +16 more
doaj +1 more source
Fermi-LAT γ-Ray Study of the Interstellar Medium and Cosmic Rays in the Chamaeleon Molecular Cloud Complex: A Look at the Dark Gas as Optically Thick H i [PDF]
Katsuhiro Hayashi +8 more
openalex +1 more source
Using the upGREAT instrument on board the Stratospheric Observatory for Infrared Astronomy, we imaged [C ii ] 157.74 and [O i ] 63.18 μ m line emission from a bright photodissociation region (PDR) associated with an ionized bubble located in the Nessie ...
James M. Jackson +17 more
doaj +1 more source
Observations of interstellar HC5N and HC7N in dark dust clouds [PDF]
L. T. Little +3 more
openaire +1 more source
The dark cloud TGU H994 P1 (LDN 1399, LDN 1400, and LDN 1402): Interstellar extinction and distance [PDF]
V. Straižys +7 more
openalex +1 more source

