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9 - Physics

Keele University

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Output 22 of 43 in the submission

Article title

Line-profile tomography of exoplanet transits - II. A gas-giant planet transiting a rapidly rotating A5 star star

Type

D - Journal article

DOI

10.1111/j.1365-2966.2010.16922.x

Title of journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Article number

Volume number

407

Issue number

First page of article

507

ISSN of journal

0035-8711

Year of publication

2010

URL

http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=000281140900042&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=65c2c6c1224a08d1a3198315ff59119e

Number of additional authors

Additional information

Smalley is a key member of the WASP project, using his expertise in stellar parameter determination to contribute tools for planet-candidate selection and for investigating planet host stars. Using these tools Smalley identified WASP-33 as a chemically peculiar (Am) star. Smalley's principal contribution the paper was the investigation into the nature of this Am star, including the spectroscopic analysis, thus confirming that this is the first planet to be identified orbiting a chemically peculiar (Am) host star, and the first hot Jupiter found to transit an A star.

Interdisciplinary

Cross-referral requested

Research group

None

Citation count

Proposed double-weighted

Double-weighted statement

Reserve for a double-weighted output

Non-English

English abstract