Results 111 to 120 of about 5,560 (224)
Cyclic C4+ as the Carrier of the Diffuse Interstellar Band at 503.9 nm?
The diffuse interstellar bands (DIBs) have remained a mystery in astronomy since their discovery over a century ago. The only currently known carrier is ${{\rm{C}}}_{60}^{+}$ , responsible for five DIBs, while more than 550 are yet to be interpreted. The
Serge. A. Krasnokutski +7 more
doaj +1 more source
Aliphatic hydrocarbon content of interstellar dust
There is considerable uncertainty as to the amount of carbon incorporated in interstellar dust. The aliphatic component of the carbonaceous dust is of particular interest because it produces a significant 3.4 mu m absorption feature when viewed against a
Schmidt, TW ; https://orcid.org/ +24 more
core +1 more source
The influence of cosmic rays on the 3.4 microns interstellar absorption band
IAU Symposium 280, Poster 37, Session 3.International audienceA 3.4 μm absorption band, assigned to aliphatic C-H stretching modes of hydrogenated amorphous carbons (a-C:H), is widely observed in diffuse interstellar medium (ISM), but the only absorption
d'Hendecourt, L. +10 more
core
The structure and properties of the diffuse interstellar medium (ISM) on small scales, sub-au to 1 pc, are poorly understood. We compare interstellar absorption-lines, observed towards a selection of O- and B-type stars at two or more epochs, to search ...
Lambert, David L. +8 more
core +1 more source
We present some of the first infrared spectral maps acquired by SPHEREx. These maps, which to our knowledge are the largest of their type ever compiled in the near-infrared, reveal multiple strong lines due to interstellar ices and polycyclic aromatic ...
Joseph L. Hora +34 more
doaj +1 more source
Distance to the Galactic Center 7′ Halo from H I Absorption
Using archival data, we have made an H I absorption study of the 7 ${}^{{\prime} }$ halo surrounding the Sgr A complex, observed toward the Galactic center (GC) region. We find strong H I absorption near velocities of −53 km s ^−1 , which is due to the 3
Debangan Maji, Subhashis Roy
doaj +1 more source
Toward a 2D H I Map of the Local Interstellar Medium
Obtaining a complete census of gas in the local interstellar medium (LISM;
Allison Youngblood +11 more
doaj +1 more source
First identified in 1964, inverse Raman scattering (IRS) is a nonlinear stimulated phenomenon that induces Raman-scattered absorptions where Raman emissions would be expected.
Frédéric Zagury
doaj +1 more source
Interstellar X-ray Absorption and Scattering
Accurate estimates of the absorption of X-rays by interstellar gas and dust are of crucial importance for the analysis and interpretation of almost all astronomical soft X-ray observations. However, the present X-ray absorption data extensively used by the community were derived from a reduced interstellar abundance (~70% of solar) and ignoring dust ...
Yan, Linli, Li, Aigen, Lu, Fangjun
openaire +2 more sources
Optical Interstellar Absorption Features [PDF]
W. Buscombe, P. M. Kennedy
openaire +1 more source

