▪ Abstract Our understanding of the evolution of organic molecules, and their voyage from
molecular clouds to the early solar system and Earth, has changed dramatically …

Molecular absorption and emission bands dominate the visible, infrared, and submillimeter
spectra of most objects with associated gas. These observations reveal a surprisingly rich …

We establish correlations between equivalent widths of eight diffuse interstellar bands
(DIBs), and examine their correlations with atomic hydrogen, molecular hydrogen, and EB …

Recently, the presence of fullerenes in the interstellar medium (ISM) has been confirmed
and new findings suggest that these fullerenes may possibly form from polycyclic aromatic …

We discuss the proposal relating the origin of some of the diffuse interstellar bands (DIBs) to
neutral and ionized polycyclic aromatic hydrocarbons (PAHs) present in interstellar clouds …

Aiming for a new and more comprehensive DIB catalog between 4000 and 9000 Å, we
revisited the Atlas Catalog based on the observations of HD 183143 and HD 204827 …

We map the distribution and properties of the Milky Way's interstellar medium as traced by
diffuse interstellar bands (DIBs) detected in near-infrared stellar spectra from the SDSS …

Aims. We study the effects of local environmental conditions affecting the diffuse interstellar
band (DIB) carriers within the Upper Scorpius subgroup of the Sco OB2 association. The aim …

Context. Diffuse interstellar bands (DIBs) are common interstellar absorption features in
spectroscopic observations but their origins remain unclear. DIBs play an important role in …

We use star, galaxy and quasar spectra taken by the Sloan Digital Sky Survey to map out the
distribution of diffuse interstellar bands (DIBs) induced by the Milky Way. After carefully …