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ALMA reveals sunburn: CO dissociation around AGB stars in the globular cluster 47 Tucanae
Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England..
Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England..
Cornell Univ, Cornell Ctr Astrophys & Planetary Sci, Ithaca, NY 14853 USA.;Observ Cote dAzur, F-06304 Nice 4, France..
Cornell Univ, Cornell Ctr Astrophys & Planetary Sci, Ithaca, NY 14853 USA..
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2015 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 453, no 4, 4324-4336 p.Article in journal (Refereed) Published
Abstract [en]

Atacama Large Millimetre Array observations show a non-detection of carbon monoxide around the four most luminous asymptotic giant branch (AGB) stars in the globular cluster 47 Tucanae. Stellar evolution models and star counts show that the mass-loss rates from these stars should be similar to 1.2-3.5x10(-7) M-circle dot yr(-1). We would naively expect such stars to be detectable at this distance (4.5 kpc). By modelling the ultraviolet radiation field from post-AGB stars and white dwarfs in 47 Tuc, we conclude that CO should be dissociated abnormally close to the stars. We estimate that the CO envelopes will be truncated at a few hundred stellar radii from their host stars and that the line intensities are about two orders of magnitude below our current detection limits. The truncation of CO envelopes should be important for AGB stars in dense clusters. Observing the CO (3-2) and higher transitions and targeting stars far from the centres of clusters should result in the detections needed to measure the outflow velocities from these stars.

Place, publisher, year, edition, pages
2015. Vol. 453, no 4, 4324-4336 p.
Keyword [en]
stars: AGB and post-AGB, circumstellar matter, stars: mass-loss, stars: winds, outflows, globular clusters: individual: NGC 104, infrared: stars
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-267651DOI: 10.1093/mnras/stv1968ISI: 000363651600071OAI: oai:DiVA.org:uu-267651DiVA: diva2:874492
Available from: 2015-11-27 Created: 2015-11-25 Last updated: 2017-12-01Bibliographically approved

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Ramstedt, Sofia

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