Results 111 to 120 of about 1,336 (203)
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 and Their Families
Diffuse interstellar bands (DIBs) still await an explanation. One expects that some progress in this field will be possible when all the known DIBs are divided into families in such a way that only one carrier is responsible for all bands belonging to the given family.
openaire +2 more sources
Interstellar Lines and Diffuse Bands in the Spectrum of the Supergiant κ Cas
© 2019, Pleiades Publishing, Ltd. We have studied the interstellar lines and diffuse bands in the spectrum of the supergiant κ Cas using the CCD spectra obtained with the Echelle spectrograph of the 2 meter telescope at the peak Terskol observatory.
Shimansky V., Rzaev A., Rza K.
core
Probing the Local Bubble with diffuse interstellar bands
Context. The Sun traverses a low-density, hot entity called the Local Bubble. Despite its relevance to life on Earth, the conditions in the Local Bubble and its exact configuration are not very well known. Besides that, there is some unknown interstellar
Jacco Th. van Loon +13 more
core +1 more source
The interpretation of the more than 300 diffuse interstellar bands (DIBs) is one of the most long-standing problems in interstellar spectra since the two first bands were reported in 1921. We now predict the frequencies of 260 diffuse interstellar bands (
Holmlid, Leif,, Leif Holmlid
core +1 more source
Polycyclic Aromatic Hydrocarbons and the Diffuse Interstellar Bands
The profiles, widths and positions of the Diffuse Interstellar Bands (DIB’s) are discussed. It is shown that the carriers of the DIB’s are molecular rather than impurities in grains. Polycyclic Aromatic Hydrocarbons (PAH’s) are attractive candidates for the DIB’s, in view of their likely abundance, their extreme stability, and the fact that these ...
Zwet, G.P. van der, Allamandola, L.J.
openaire +3 more sources
Fine structure of profiles of weak diffuse interstellar bands
We present a very high resolution ($R=120\,000$–220 000) analysis of profiles of selected diffuse interstellar bands (DIBs): 4964, 4980, 4985, 5850 Å.
F. Musaev +5 more
core +1 more source
Spectroscopic families among diffuse interstellar bands
The inability to identify carriers of the diffuse interstellar bands (DIBs) is one of the longest standing problems in astronomy and astrochemistry. It is debated whether these carriers arise from dust or the gas component of the interstellar medium ...
Wszołek, B.
core +1 more source
Diffuse Interstellar Bands Toward HD 62542 [PDF]
Diffuse interstellar bands (DIBs) have been detected for the first time along the peculiar translucent line of sight toward HD 62542, which passes through a diffuse cloud core.
Blake, Geoffrey A. +2 more
core
The ESO Diffuse Interstellar Bands Large Exploration Survey: EDIBLES I. Project description, survey sample and quality assessment. [PDF]
Cox NLJ +29 more
europepmc +1 more source

