Results 111 to 120 of about 22,641 (242)
As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the large-scale diffuse gas and dust in Giant Molecular Clouds (GMCs), how it moves, how it is ...
Pamela Klaassen +40 more
doaj +1 more source
On the possible contribution of cationic oxygenated carbon chains CnO+, HCnO+, and OCnO+ (n = 4–9) to the diffuse interstellar bands [PDF]
Ugo Jacovella +5 more
openalex +1 more source
ASSIGNMENT OF 5069 Å DIFFUSE INTERSTELLAR BAND TO HC 4 H + : DISAGREEMENT WITH LABORATORY ABSORPTION BAND [PDF]
John P. Maier +6 more
openalex +1 more source
CRIRES high-resolution near-infrared spectroscopy of diffuse interstellar band profiles
A. Ebenbichler
openalex +2 more sources
The structure and chemistry of the dusty interstellar medium (ISM) are shaped by complex processes that depend on the local radiation field, gas composition, and dust grain properties. Of particular importance are polycyclic aromatic hydrocarbons (PAHs),
Dalya Baron +24 more
doaj +1 more source
New Infrared Diffuse Interstellar Bands in the Galactic Center and Elsewhere [PDF]
T. R. Geballe
openalex +1 more source
Diffuse Bands 9577 and 9633: Relations to Other Interstellar Features [PDF]
Г. А. Галазутдинов +3 more
openalex +1 more source
The Diffuse Interstellar Bands: Solving a Century Old Problem [PDF]
The Diffuse Interstellar Bands (DIBs) are a set of apporoximately 500 absorption bands that are seen in the spectra of reddened stars (i.e., stars obscured by the presence of interstellar clouds in their line of sight).
Salama, Farid
core +1 more source
Unusual relative strengths of the diffuse interstellar bands in some interstellar dust clouds [PDF]
Some of the diffuse interstellar features (DIBs) in the spectra of certain stars at high galactic latitudes (1 is greater than 15 degrees) are unusually weak or absent while others have the strength expected for their color excess.
Krelowski, J., Walker, G. A. H.
core +1 more source

