Results 111 to 120 of about 22,641 (242)

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy [version 1; peer review: 2 approved]

open access: yesOpen Research Europe
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

ASSIGNMENT OF 5069 Å DIFFUSE INTERSTELLAR BAND TO HC 4 H + : DISAGREEMENT WITH LABORATORY ABSORPTION BAND [PDF]

open access: bronze, 2011
John P. Maier   +6 more
openalex   +1 more source

PHANGS-ML: The Universal Relation between PAH Band and Optical Line Ratios across Nearby Star-forming Galaxies

open access: yesThe Astrophysical Journal
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

Diffuse interstellar bands in M 33 [PDF]

open access: bronze, 2008
Martin Cordiner   +7 more
openalex   +1 more source

Diffuse Bands 9577 and 9633: Relations to Other Interstellar Features [PDF]

open access: bronze, 2021
Г. А. Галазутдинов   +3 more
openalex   +1 more source

The Diffuse Interstellar Bands: Solving a Century Old Problem [PDF]

open access: yes
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]

open access: yes
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

Home - About - Disclaimer - Privacy