The detection of dust around NN Ser

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Abstract

Eclipse timing variations observed from the post-common-envelope binary (PCEB) NN Ser offer strong evidence in favour of circumbinary planets existing around PCEBs. If real, these planets may be accompanied by a disc of dust. We here present the ALMA detection of flux at 1.3 mm from NN Ser, which is likely due to thermal emission from a dust disc of mass ∼0.8 ± 0.2 M⊕. We performed simulations of the history of NN Ser to determine possible origins of this dust, and conclude that the most likely origin is, in fact, common-envelope material which was not expelled from the system and instead formed a circumbinary disc. These discs have been predicted by theory but previously remained undetected. While the presence of this dust does not prove the existence of planets around NN Ser, it adds credibility to the possibility of planets forming from common-envelope material in a ‘second-generation’ scenario.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science, Engineering and Medicine > Science > Physics
Library of Congress Subject Headings (LCSH): Protoplanetary disks, Eclipsing binaries
Journal or Publication Title: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press
ISSN: 0035-8711
Official Date: 23 April 2016
Dates:
Date
Event
23 April 2016
Available
20 April 2016
Accepted
19 April 2016
Submitted
Volume: 459
Number: 4
Number of Pages: 9
Page Range: pp. 4518-4526
DOI: 10.1093/mnras/stw976
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
Date of first compliant deposit: 3 June 2016
Date of first compliant Open Access: 6 June 2016
Funder: Millennium Science Initiative, Fondo Nacional de Desarrollo Científico y Tecnológico (Chile) (FONDECYT), European Research Council (ERC), Seventh Framework Programme (European Commission) (FP7), Science and Technology Facilities Council (Great Britain) (STFC)
Grant number: RC130007 (MSI), 1141269 (FONDECYT), 3140592 (FONDECYT), 3140585 (FONDECYT), 1140109 (FONDECYT), 320964 (FP7), ST/L000733 (STFC)
Adapted As:
URI: https://wrap.warwick.ac.uk/79470/

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