C - looking for the bucky-ball in interstellar space
arXiv:1612.08898 · doi:10.1093/mnras/stw2948
Abstract
The laboratory gas phase spectrum recently published by Campbell et al. has reinvigorated attempts to confirm the presence of the C cation in the interstellar medium, thorough an analysis of the spectra of hot, reddened stars. This search is hindered by at least two issues that need to be addressed: (i) the wavelength range of interest is severely polluted by strong water- vapour lines coming from the Earth's atmosphere; (ii) one of the major bands attributed to C, at 9633 Å, is blended with the stellar Mg{\sc ii} line, which is susceptible to non-local-thermodynamic equilibrium effects in hot stellar atmospheres. Both these issues are here carefully considered here for the first time, based on high-resolution and high signal-to-noise ratio echellé spectra for 19 lines of sight. The result is that the presence of C in interstellar clouds is brought into question.
arXiv comment10 pages, 11 figures
References in corpus (7)
- Molecfit: A general tool for telluric absorption correction. I. Method and application to ESO instruments
- New Grids of ATLAS9 Model Atmospheres
- C in Reflection Nebulae
- Studies of the Diffuse Interstellar Bands. III. HD 183143
- Identification of more interstellar C60+ bands
- Interstellar C60+
- Stellar modelling of Spica, a high-mass spectroscopic binary with a beta Cep variable primary component
Cited by in corpus (21)
- Confirming interstellar C using the Hubble Space Telescope
- The Apache Point Observatory Catalog of Optical Diffuse Interstellar Bands
- The ESO Diffuse Interstellar Bands Large Exploration Survey: EDIBLES I. Project description, survey sample and quality assessment
- C and the Diffuse Interstellar Bands: An Independent Laboratory Check
- Searching for interstellar C60+ using a new method for high signal-to-noise HST/STIS spectroscopy
- EDIBLES II. On the detectability of C60+ bands
- The Behavior of Selected Diffuse Interstellar Bands with Molecular Fraction in Diffuse Atomic and Molecular Clouds
- DECH: Software Package for Astronomical Spectral Data Processing and Analysis
- Are the Carriers of Diffuse Interstellar Bands and Extended Red Emission the same?
- Survey of near-infrared diffuse interstellar bands in and bands. I. Newly identified bands
- Diffuse bands 9577 and 9633 -- relations to other interstellar features
- Survey of very broad Diffuse Interstellar Bands
- C diffuse interstellar band correlations and environmental variations
- The diffuse interstellar band around 8620 Å II. Kinematics and distance of the DIB carrier
- A high resolution study of near-IR diffuse interstellar bands, search for small scale structure, time variability and stellar features
- C60 Cation as the Carrier of the 9577 and 9632 Angstrom Diffuse Interstellar Bands: Further Support from the VLT/X-Shooter Spectra
- The C60:C60+ ratio in diffuse and translucent interstellar clouds
- Near-Infrared Diffuse Interstellar Bands towards Her 36
- Broadened profiles of Diffuse Interstellar Bands
- Analysis of integrated-light spectra of Galactic globular clusters
- The Pristine Inner Galaxy Survey (PIGS) VI: Different vertical distributions between two DIBs at 442.8 nm and 862.1 nm