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
Sheets H
(2013)
DUSTY OB STARS IN THE SMALL MAGELLANIC CLOUD. I. OPTICAL SPECTROSCOPY REVEALS PREDOMINANTLY MAIN-SEQUENCE OB STARS
in The Astrophysical Journal
Turner T
(2011)
X-RAY CHARACTERISTICS OF NGC 3516: A VIEW THROUGH THE COMPLEX ABSORBER
in The Astrophysical Journal
Volk K
(2011)
DISCOVERY AND ANALYSIS OF 21 µm FEATURE SOURCES IN THE MAGELLANIC CLOUDS
in The Astrophysical Journal
Markowitz A
(2009)
ASUZAKUOBSERVATION OF NGC 4593: ILLUMINATING THE TRUNCATED DISK
in The Astrophysical Journal
Boyer M
(2009)
DUST PRODUCTION AND MASS LOSS IN THE GALACTIC GLOBULAR CLUSTER NGC 362
in The Astrophysical Journal
Sloan G
(2012)
CARBON-RICH DUST PRODUCTION IN METAL-POOR GALAXIES IN THE LOCAL GROUP
in The Astrophysical Journal
Sandstrom K
(2012)
THE SPITZER SPECTROSCOPIC SURVEY OF THE SMALL MAGELLANIC CLOUD (S 4 MC): PROBING THE PHYSICAL STATE OF POLYCYCLIC AROMATIC HYDROCARBONS IN A LOW-METALLICITY ENVIRONMENT
in The Astrophysical Journal
Southworth J
(2009)
PHYSICAL PROPERTIES OF THE 0.94-DAY PERIOD TRANSITING PLANETARY SYSTEM WASP-18
in The Astrophysical Journal
Risaliti G
(2009)
VARIABLE PARTIAL COVERING AND A RELATIVISTIC IRON LINE IN NGC 1365
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
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 |