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The EDIBLES survey
- Source :
- Astronomy and Astrophysics, Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 616, pp.A143. ⟨10.1051/0004-6361/201833105⟩, Astronomy and Astrophysics, 616, A143
- Publication Year :
- 2018
- Publisher :
- EDP Sciences, 2018.
-
Abstract
- The so-called C2-DIBs are a class of very weak bands that fall in the blue part of the optical spectrum and are associated with high column densities of the C2 molecule. DIB profile structures constrain potential molecular carriers, but their measurement requires high S/N and spectra and the use of sightlines without Doppler splitting, as typical for a single-cloud situation. Spectra from the ESO Diffuse Interstellar Bands Large Exploration Survey (EDIBLES) conducted at the VLT (ESO/Paranal) were explored to identify single-cloud and high C2 column sightlines, extract the corresponding C2-DIBs and study their strengths and profiles, and to investigate in detail any sub-structures. The target selection was made based on profile-fitting of the Sodium doublets and the detection of C2 lines. The C2 (2-0) Phillips system was fitted using a physical model of the host cloud. C2 column densities, temperatures as well as gas densities were derived for each sightline. 18 known C2-DIBs and 8 strong non-C2 DIBs were extracted towards 8 targets, comprising 7 single-cloud and one multi-cloud line-of-sights. Correlational studies revealed a tight association of the former group with the C2 columns, whereas the non-C2 DIBs are primarily correlated with reddening. We report three new weak diffuse band candidates. We show for the first time that at least 14 C2-DIBs exhibit spectral sub-structures which are consistent with unresolved rotational branches of molecular carriers. The variability of their peak separations among the bands for a given sightline implies that their carriers are different molecules with quite different sizes. We also illustrate how profiles of the same DIB vary among targets and as a function of physical parameters and provide tables defining the sub-structures to be compared with future models and experimental results.<br />19 pages, 15 figures, accepted for publication in A&A
- Subjects :
- [PHYS]Physics [physics]
Physics
Very Large Telescope
Diffuse interstellar band
FOS: Physical sciences
line: profiles
Astronomy and Astrophysics
Context (language use)
Astrophysics
Astrophysics - Astrophysics of Galaxies
ISM: clouds
01 natural sciences
ISM: molecules
Spectral line
Interstellar medium
symbols.namesake
Space and Planetary Science
Astrophysics of Galaxies (astro-ph.GA)
0103 physical sciences
symbols
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
010306 general physics
010303 astronomy & astrophysics
Doppler effect
Subjects
Details
- ISSN :
- 14320746 and 00046361
- Volume :
- 616
- Database :
- OpenAIRE
- Journal :
- Astronomy & Astrophysics
- Accession number :
- edsair.doi.dedup.....910720b1b9350d180d01a372a98a9cd3
- Full Text :
- https://doi.org/10.1051/0004-6361/201833105