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.
Organisations
Publications
Bonanos A
(2010)
The Infrared Properties of Massive Stars in the Magellanic Clouds
Faedi F
(2016)
WASP-86b and WASP-102b: super-dense versus bloated planets
Thielemann F
(2011)
Astronomy with Radioactivities
{Jones}, S. And {Hirschi}, R. And {Herwig}, F. And {Paxton}, B. And {Timmes}, F.~X. And {Nomoto}, K.
(2012)
Progenitors of electron-capture supernovae
Faedi F
(2016)
WASP-86b and WASP-102b: super-dense versus bloated planets
Maxted P. F. L.
(2016)
VizieR Online Data Catalog: ellc: a fast, flexible light curve model (Maxted, 2016)
in VizieR Online Data Catalog
Maxted P. F. L.
(2016)
VizieR Online Data Catalog: Five transiting hot Jupiters discovered using WASP (Maxted+, 2016)
in VizieR Online Data Catalog
Maxted P. F. L.
(2016)
VizieR Online Data Catalog: Five transiting hot Jupiters discovered using WASP (Maxted+, 2016)
in VizieR Online Data Catalog
Lendl M.
(2016)
VizieR Online Data Catalog: WASP-49b FORS2 multi-epoch spectra (Lendl+, 2016)
in VizieR Online Data Catalog
McDonald I
(2011)
FUNDAMENTAL PARAMETERS, INTEGRATED RED GIANT BRANCH MASS LOSS, AND DUST PRODUCTION IN THE GALACTIC GLOBULAR CLUSTER 47 TUCANAE
in The Astrophysical Journal Supplement Series
Ferrarese L
(2012)
THE NEXT GENERATION VIRGO CLUSTER SURVEY (NGVS). I. INTRODUCTION TO THE SURVEY*
in The Astrophysical Journal Supplement Series
Jordán A
(2013)
A GROUND-BASED OPTICAL TRANSMISSION SPECTRUM OF WASP-6b
in The Astrophysical Journal
Wilson D
(2008)
WASP-4b: A 12th Magnitude Transiting Hot Jupiter in the Southern Hemisphere
in The Astrophysical Journal
Indebetouw R
(2013)
ALMA RESOLVES 30 DORADUS: SUB-PARSEC MOLECULAR CLOUD STRUCTURE NEAR THE CLOSEST SUPER STAR CLUSTER
in The Astrophysical Journal
Volk K
(2011)
ERRATUM: "DISCOVERY AND ANALYSIS OF 21 µm FEATURE SOURCES IN THE MAGELLANIC CLOUDS" (2011, ApJ, 735, 127)
in The Astrophysical Journal
Reeves J
(2009)
A COMPTON-THICK WIND IN THE HIGH-LUMINOSITY QUASAR, PDS 456
in The Astrophysical Journal
Bolatto A
(2011)
THE STATE OF THE GAS AND THE RELATION BETWEEN GAS AND STAR FORMATION AT LOW METALLICITY: THE SMALL MAGELLANIC CLOUD
in The Astrophysical Journal
Shin I
(2012)
CHARACTERIZING LOW-MASS BINARIES FROM OBSERVATION OF LONG-TIMESCALE CAUSTIC-CROSSING GRAVITATIONAL MICROLENSING EVENTS
in The Astrophysical Journal
Lawton B
(2010)
SPITZER ANALYSIS OF H II REGION COMPLEXES IN THE MAGELLANIC CLOUDS: DETERMINING A SUITABLE MONOCHROMATIC OBSCURED STAR FORMATION INDICATOR
in The Astrophysical Journal
Hellier C
(2011)
ON THE ORBIT OF THE SHORT-PERIOD EXOPLANET WASP-19b
in The Astrophysical Journal
Pignatari M
(2013)
PRODUCTION OF CARBON-RICH PRESOLAR GRAINS FROM MASSIVE STARS
in The Astrophysical Journal
| 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 |