Behaviour of the Broadest DIBs as a Function of E(B–V). Issue Volume 9:Issue S297(2013) (21st February 2014)

• Record Type: Journal Article
• Authors: York, B.; Sonnentrucker, P.; Hobbs, L. M.; York, D. G.; Friedman, S. D.; Dahlstrom, J.; Welty, D. E.; Snow, T. P.; Rachford, B. L.
• Is Part Of: Proceedings of the International Astronomical Union. Volume 9:Issue S297(2013)
• Page Start: 138
• Page End: 140
• Publication Date: 2014-02-21
• Subjects: ISM: lines and bands; Astronomy -- Congresses; Astronomy -- Periodicals; 520
• DOI: 10.1017/S1743921313015767
• Languages: English
• ISSNs: 1743-9213

Abstract

Abstract: We present the first results of a dedicated search for Diffuse Interstellar Bands that have profiles with FWHM > 6 Å. Broad DIBs have been noticed in past surveys using averages of multiple sight lines (e.g. Jenniskens & Désert, 1994), but careful detection, measurement, and cataloguing for individual sight lines has not been done since the pioneering work of Herbig (1995). We have initiated an observing campaign using the Apache Point Observatory in order to obtain low-resolution spectra to search for such broad DIBs and monitor their behaviour from star to star. A first sample of 21 stars with 0.3 < E(B-V) < 3.3 mag, along with 15 matched low-reddening stars, were observed with the APO/DIS B400 (R ~ 450) and R300 (R ~ 1000) gratings to obtain spectra having S/N > 500.