Stellar Astrophysics at Keele

Lead Research Organisation: Keele University
Department Name: Sch of Chemistry & Physics

Abstract

Our home is a planet orbiting a star. To understand our origins and place in the universe we need to understand how planets and stars form. Using a novel sky-survey instrument, which we are building in South Africa, we will search for planets around other stars. Using the latest and biggest telescopes and satellites we will study stellar nurseries where stars are born. We will investigate how they evolve, how they interact with each other, how they interact with their environment, and how they enrich interstellar space with the chemical ingredients from which a new generation of stars and planets will form, and from which, ultimately, we ourselves are made.

Publications

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Copperwheat C (2011) SDSS J0926+3624: the shortest period eclipsing binary star The shortest period eclipsing binary star in Monthly Notices of the Royal Astronomical Society

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Kane S (2008) SuperWASP-N extrasolar planet candidates from fields 06 h < RA < 16 h in Monthly Notices of the Royal Astronomical Society

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Rushton M (2008) How peculiar is the â??peculiar variableâ?? DZ Crucis (Nova Cru 2003)? in Monthly Notices of the Royal Astronomical Society

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Groenewegen M (2007) Luminosities and mass-loss rates of carbon stars in the Magellanic Clouds in Monthly Notices of the Royal Astronomical Society

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Jeffries R (2009) Low-mass members of the young cluster IC 4665 and pre-main-sequence lithium depletion in Monthly Notices of the Royal Astronomical Society

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Jackson R (2013) On the relationship between the size and surface coverage of starspots on magnetically active low-mass stars in Monthly Notices of the Royal Astronomical Society

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Christian D (2007) Erratum: The Super WASP wide-field exoplanetary transit survey: candidates from fields 23 h < RA < 03 h in Monthly Notices of the Royal Astronomical Society

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Maxted P (2013) Spitzer 3.6 and 4.5 µm full-orbit light curves of WASP-18 in Monthly Notices of the Royal Astronomical Society

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Doyle A (2013) Accurate spectroscopic parameters of WASP planet host stars? in Monthly Notices of the Royal Astronomical Society

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Miller L (2010) X-ray reverberation in 1H 0707-495 revisited X-ray reverberation in 1H 0707-495 in Monthly Notices of the Royal Astronomical Society

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Oliveira J (2006) Massive young stellar objects in the Large Magellanic Cloud: water masers and ESO-VLT 3-4  m spectroscopy in Monthly Notices of the Royal Astronomical Society

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Unda-Sanzana E (2008) GD 552: a cataclysmic variable with a brown dwarf companion? in Monthly Notices of the Royal Astronomical Society

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Braito V (2013) Decoupling absorption and continuum variability in the Seyfert 2 NGC 4507 in Monthly Notices of the Royal Astronomical Society

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Southworth J (2012) Refined physical properties of the HAT-P-13 planetary system Physical properties of HAT-P-13 in Monthly Notices of the Royal Astronomical Society

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Brown D (2011) Are falling planets spinning up their host stars? Are falling planets spinning up their host stars? in Monthly Notices of the Royal Astronomical Society

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Jeffries R (2006) An XMM-Newton observation of the young open cluster NGC 2547: coronal activity at 30 Myr in Monthly Notices of the Royal Astronomical Society

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Binks A (2013) A lithium depletion boundary age of 21 Myr for the Beta Pictoris moving group in Monthly Notices of the Royal Astronomical Society: Letters

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Oliveira J (2011) Ice chemistry in massive young stellar objects: the role of metallicity in Monthly Notices of the Royal Astronomical Society: Letters

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Jeffries R (2006) Kinematic structure in the young s Orionis association in Monthly Notices of the Royal Astronomical Society: Letters

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Jackson R (2009) The radii of M-dwarfs in the young open cluster NGC 2516 in Monthly Notices of the Royal Astronomical Society: Letters

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Anderson D (2008) WASP-5b: a dense, very hot Jupiter transiting a 12th-mag Southern-hemisphere star in Monthly Notices of the Royal Astronomical Society: Letters

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Reeves J (2008) On why the iron K-shell absorption in AGN is not a signature of the local warm/hot intergalactic medium in Monthly Notices of the Royal Astronomical Society: Letters

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Miller L (2009) The absorption-dominated model for the X-ray spectra of type I active galaxies: MCG-6-30-15 in Monthly Notices of the Royal Astronomical Society: Letters

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Tombesi F (2011) X-ray evidence for the accretion disc-outflow connection in 3C 111 Accretion disc-outflow connection in 3C 111 in Monthly Notices of the Royal Astronomical Society: Letters

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Gänsicke B (2008) SDSS J084539.17+225728.0: the first DBZ white dwarf with a metal-rich gaseous debris disc in Monthly Notices of the Royal Astronomical Society: Letters

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Tombesi F (2012) Evidence for ultrafast outflows in radio-quiet AGNs - III. Location and energetics in Monthly Notices of the Royal Astronomical Society: Letters

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Evans A (2012) Solid-phase C60 in the peculiar binary XX Oph? C60 in XX Oph in Monthly Notices of the Royal Astronomical Society: Letters

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Burleigh M (2006) A near-infrared spectroscopic detection of the brown dwarf in the post common envelope binary WD 0137-349 in Monthly Notices of the Royal Astronomical Society: Letters

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Littlefair S (2011) Accretion-induced luminosity spreads in young clusters: evidence from stellar rotation in Monthly Notices of the Royal Astronomical Society: Letters

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Risaliti G (2009) The XMM-Newton long look of NGC 1365: uncovering of the obscured X-ray source in Monthly Notices of the Royal Astronomical Society: Letters

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Evans A (2006) The Spitzer Infrared Spectrometer view of V4334 Sgr (Sakurai's Object) in Monthly Notices of the Royal Astronomical Society: Letters

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Southworth John (2012) ASTRONOMY A new class of planet in NATURE

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Hirschi R. (2006) GRB progenitors at low metallicities in NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-BASIC TOPICS IN PHYSICS

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Yonetoku D. (2006) Suzaku observation of X-ray afterglow: Spectral and temporal behaviors in NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS

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Van Loon J (2010) Chemical evolution of star clusters in Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences

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Van Loon JT (2010) Chemical evolution of star clusters. in Philosophical transactions. Series A, Mathematical, physical, and engineering sciences

 
Description Lots and lots of them 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? No
Geographic Reach National
Primary Audience Media (as a channel to the public)
Results and Impact We have particpated in dozens and dozens of such activites.

Lots. We have about dozens and dozens of such feedbacks.
Year(s) Of Engagement Activity Pre-2006,2006,2007,2008,2009,2010,2011,2012,2013,2014