We report a deep survey of diffuse interstellar bands (DIBs) between 3906 Angstrom and 6812 Angstrom under consistent observing conditions toward three very reddened and five unreddened stars. BD+63 degrees 1964\u27s line-of-sight was shown to present exceptional DIB enhancement in number as well as in strength. The early spectral type of the star and the use of spectra of an unreddened comparison star of the same spectral type allowed to limit stellar line residuals. Using careful reduction and analysis methods we discovered 60 new DIBs which are confirmed in the reddened targets HD 183143 and BD+40 degrees 4220. We detected 25 possible DIBs which still await further confirmation, but we did not detect or confirm 28 previously reported DIB...
The diffuse interstellar bands (DIBs) are absorption lines observed in visual and near-infrared spec...
Author Institution: University of Chicago, Yerkes Observatory, Williams Bay, WI 53191; University of...
Context. The diffuse interstellar bands (DIBs) are a set of hundreds of unidentified absorption feat...
We report a deep survey of diffuse interstellar bands (DIBs) between 3906 Angstrom and 6812 Angstrom...
We report a deep survey of diffuse interstellar bands (DIBs) between 3906 Å and 6812 Åunder consist...
Echelle spectra of HD 183143 [B7Iae, E(B − V) = 1.27] were obtained on three nights, at a resolving...
We have used spectra of hot stars from the RAVE Survey in order to investigate the visibility and pr...
Diffuse interstellar bands (DIBs) have been discovered for almost a century, but their nature remain...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
We have used spectra of hot stars from the RAVE Survey in order to investigate the visibility and pr...
Aims. Stellar spectroscopic surveys may bring useful statistical information on the links between di...
The diffuse interstellar bands (DIBs) are absorption lines observed in visual and near-infrared spec...
Author Institution: University of Chicago, Yerkes Observatory, Williams Bay, WI 53191; University of...
Context. The diffuse interstellar bands (DIBs) are a set of hundreds of unidentified absorption feat...
We report a deep survey of diffuse interstellar bands (DIBs) between 3906 Angstrom and 6812 Angstrom...
We report a deep survey of diffuse interstellar bands (DIBs) between 3906 Å and 6812 Åunder consist...
Echelle spectra of HD 183143 [B7Iae, E(B − V) = 1.27] were obtained on three nights, at a resolving...
We have used spectra of hot stars from the RAVE Survey in order to investigate the visibility and pr...
Diffuse interstellar bands (DIBs) have been discovered for almost a century, but their nature remain...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
We have used spectra of hot stars from the RAVE Survey in order to investigate the visibility and pr...
Aims. Stellar spectroscopic surveys may bring useful statistical information on the links between di...
The diffuse interstellar bands (DIBs) are absorption lines observed in visual and near-infrared spec...
Author Institution: University of Chicago, Yerkes Observatory, Williams Bay, WI 53191; University of...
Context. The diffuse interstellar bands (DIBs) are a set of hundreds of unidentified absorption feat...