Carbon monoxide emission from young planetary nebulae

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Other literature type 01 Jan 1989 English Publisher:Springer Berlin HeidelbergJournal:International Astronomical Union Colloquium, volume 120, pages 193-193 (issn: 0252-9211,

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Authors: R. Bachiller; V. Bujarrabal; J. Martín-Pintado; P. Planesas; J. Gómez-González;

doi: 10.1007/bfb0114865 , 10.1017/s0252921100023721

Carbon monoxide emission from young planetary nebulae

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Abstract

We have mapped the CO J=2-l and J=l-0 emission with high angular resolution (about 10” and 20”, respectively) from the young planetary nebulae NGC2346, M2-9 and NGC6720 (the Ring nebula in Lyra). The observations were carried out by using the IRAM 30-m dish at Pico Veleta (near Granada, Spain).

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Yebes Observatory
Spain

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