Results 101 to 110 of about 22,641 (242)

A search for diffuse bands in fullerene planetary nebulae: evidence of diffuse circumstellar bands

open access: yes, 2014
Large fullerenes and fullerene-based molecules have been proposed as carriers of diffuse interstellar bands (DIBs). The recent detection of the most common fullerenes (C60 and C70) around some planetary nebulae (PNe) now enable us to study the DIBs ...
Cataldo, F.   +4 more
core   +1 more source

TheGaia-ESO Survey: Extracting diffuse interstellar bands from cool star spectra [PDF]

open access: bronze, 2014
L. Puspitarini   +27 more
openalex   +1 more source

Diffuse interstellar bands in the H II region M17 [PDF]

open access: bronze, 2018
M. C. Ramírez-Tannus   +3 more
openalex   +1 more source

The Multiwavelength Extinction Law and Its Variation in the Coalsack Molecular Cloud Based on the Gaia, APASS, SMSS, 2MASS, GLIMPSE, and WISE Surveys

open access: yesThe Astrophysical Journal
Accurate interpretation of observations relies on the interstellar dust extinction law, which also serves as a powerful diagnostic for probing dust properties.
Juan Deng   +3 more
doaj   +1 more source

The diffuse interstellar band around 8620 Å [PDF]

open access: hybrid, 2020
H. Zhao   +8 more
openalex   +1 more source

Where Have All the Sulfur Atoms Gone? Polycyclic Aromatic Hydrocarbon as a Possible Sink for the Missing Sulfur in the Interstellar Medium. I. The C–S Band Strengths

open access: yesThe Astrophysical Journal
Despite its biogenic and astrochemical importance, sulfur (S), the 10th most abundant element in the interstellar medium (ISM) with a total abundance of S/H ≈ 2.2 × 10 ^−5 , largely remains undetected in molecular clouds.
X. J. Yang, Lijun Hua, Aigen Li
doaj   +1 more source

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy [version 2; 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

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