By L. Hartmann (auth.), G. D. Watt, P. M. Williams (eds.)
The convention recorded during this quantity was once one of many occasions organised to have fun the centenary of the (re)establishment of the Royal Observatory, Edinburgh, on Blackford Hill in 1884. Circumstellar topic used to be chosen because the subject due to very important contributions towards examine within the box by way of fresh observations within the infrared and submillimetre, relatively with the 2 telescopes which the Observatory has either operated and outfitted instru mentation for - the uk Infrared Telescope (UKIRT) and the James Clerk Maxwell Telescope (JCMT). The programme aimed to hide as many points of circumstellar subject as may perhaps healthy right into a one-week assembly, omitting in simple terms planetary nebulae, which were good served through conferences within the past years. We thank the overseas medical advisory com mittee (overleaf) for his or her assist in settling on the Invited Reviewers round which the programme used to be outfitted. The Invited experiences and oral contributions are integrated within the order and sections within which they have been provided, even the place re-ordering could have been extra logical. We didn't try to categorise the poster contributions yet have incorporated them in alphabetical order. a night consultation for viewing and discussing posters in an unhurried surroundings was once very profitable. a contest for the simplest poster was once held and the prize was once offered for that by way of Lindqvist, Lucas, Olofsson, Omont, Eriksson & Gustafsson.
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Extra info for Circumstellar Matter 1994: Proceedings of an International Conference to Celebrate the Centenary of the Royal Observatory, Edinburgh, held at the Edinburgh Conference Centre, Heriot-Watt University, Riccarton, Edinburgh, Scotland, 29 August – 2 September,
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Autonoma de Madrid Abstract. We present a study of weak near-IR absorption lines in 44 low luminosity YSOs. Using a spectral resolution of rv 1000 most Class II sources show CO overtone absorption bands of varying strength in the K window, whether they have optical counterparts or not. Class I sources tend to show featureless 2 I'm continua even though a SIN> 100 was achieved. High resolution (R=17000) echelle spectra were also obtained for a sub-sample of YSOs. Most show an unresolved 12CO(2-0) bandhead, which when combined with inferred CO excitation temperatures and optical depths clearly points to a photospheric rather than a disk origin for the bands.
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