Open University Consolidated Grant Phase 1
Lead Research Organisation:
The Open University
Department Name: Physical Sciences
Abstract
We will study a wide range of some of the most important problems in modern astrophysics. Our programme is aimed at: a) Measuring the make-up and composition of the basic components of material in our Galaxy. This includes understanding where energetic 'cosmic ray' particles in the space between stars come from; studying the birth and evolution of massive stars from observations of placental ionised birthplaces (called HII regions) using LOFAR, STFC's new radio telescope; examining how young massive star clusters influence their local region of space via their UV radiation, and how they deposit material and mechanical energy back into space. Finally, to understand how some massive stars quite quickly form massive stellar remnants, such as black holes. b) We will study exoplanets, planets orbiting around distant stars. We will observe the structure and properties of their atmospheres, to learn whether close-in planets are consumed by their host star. We are working towards detecting habitable exoplanets, including examining whether we can identify systems with rocky planets using the chemical composition of the host star's atmosphere. We are also studying the rocky planets in the Solar System: to understand the water and dust cycles in in the Martian atmosphere and the contributions of atmospheric eddy processes in the atmosphere of Venus. c) On a much larger scale, we seek to understand the structure and history of the entire Universe: studying the dark matter distribution in giant galaxies, and understanding how black hole accretion affects star formation; and using data from the Herschel and ground based telescopes, assessing the physical and morphological properties of distant star-forming galaxies, and studying how the evolving energy budget of the Universe. d) Experimenting in the laboratory to mimic the formation of molecules in on dust grains in space that lead to the complex chemistry that acted as the precursor to life in the Universe, and to explore the chemistry of Mars and Titan. e) Finally, we propose developing and extending our unique programme of Public Engagement and Outreach, to bring the excitement of the Universe to the general public, and the next generation of young people.
Planned Impact
Attached as a separate document, and also included as Appendix D in the main case
Organisations
Publications
Arab H
(2012)
Evolution of dust in the Orion Bar with Herschel I. Radiative transfer modelling
in Astronomy & Astrophysics
Asgekar A
(2013)
LOFAR detections of low-frequency radio recombination lines towards Cassiopeia A
in Astronomy & Astrophysics
Bernard-Salas J
(2012)
Spatial variation of the cooling lines in the Orion Bar from Herschel /PACS
in Astronomy & Astrophysics
Bloom J
(2012)
A COMPACT DEGENERATE PRIMARY-STAR PROGENITOR OF SN 2011fe
in The Astrophysical Journal
Buckle J
(2012)
The JCMT Legacy Survey of the Gould Belt: mapping 13CO and C18O in Orion A GBS HARP survey: Orion A
in Monthly Notices of the Royal Astronomical Society
Cappetta M
(2012)
The first planet detected in the WTS: an inflated hot Jupiter in a 3.35 d orbit around a late F star Inflated HJ in close orbit around a late-F-star
in Monthly Notices of the Royal Astronomical Society
Christie H
(2012)
CO depletion in the Gould Belt clouds CO depletion in the Gould Belt clouds
in Monthly Notices of the Royal Astronomical Society
Davies B
(2012)
The G305 star-forming complex: the central star clusters Danks 1 and Danks 2 The young star clusters Danks 1 and Danks 2
in Monthly Notices of the Royal Astronomical Society
Dent W
(2013)
GASPS-A Herschel Survey of Gas and Dust in Protoplanetary Disks: Summary and Initial Statistics
in Publications of the Astronomical Society of the Pacific
Doi Y
(2012)
AKARI FAR-INFRARED ALL-SKY SURVEY MAPS
in Publications of The Korean Astronomical Society
Eiroa C
(2013)
DUst around NEarby Stars. The survey observational results
in Astronomy & Astrophysics
Enoch B
(2012)
Transit algorithm performance using real WASP data
in Astronomy & Astrophysics
Ertel S
(2012)
A peculiar class of debris disks from Herschel /DUNES A steep fall off in the far infrared
in Astronomy & Astrophysics
Ertel S
(2014)
Potential multi-component structure of the debris disk around HIP 17439 revealed by Herschel /DUNES
in Astronomy & Astrophysics
Faedi F
(2013)
WASP-54b, WASP-56b, and WASP-57b: Three new sub-Jupiter mass planets from SuperWASP
in Astronomy & Astrophysics
Fallscheer C
(2013)
HERSCHEL REVEALS MASSIVE COLD CLUMPS IN NGC 7538
in The Astrophysical Journal
Faramaz V
(2014)
Can eccentric debris disks be long-lived? A first numerical investigation and application to ? 2 Reticuli???
in Astronomy & Astrophysics
Farmer R
(2013)
The true stellar parameters of the Kepler target list
in Monthly Notices of the Royal Astronomical Society
Fossati L
(2012)
THE HABITABILITY AND DETECTION OF EARTH-LIKE PLANETS ORBITING COOL WHITE DWARFS
in The Astrophysical Journal
Fujiwara H
(2013)
AKARI/IRC 18 µ m survey of warm debris disks
in Astronomy & Astrophysics
Giannini T
(2012)
The Herschel view of the on-going star formation in the Vela-C molecular cloud
in Astronomy & Astrophysics
Giesting P
(2015)
Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes
in Meteoritics & Planetary Science
Gómez Maqueo Chew Y
(2013)
Discovery of WASP-65b and WASP-75b: Two hot Jupiters without highly inflated radii
in Astronomy & Astrophysics
Haswell C
(2012)
NEAR-ULTRAVIOLET ABSORPTION, CHROMOSPHERIC ACTIVITY, AND STAR-PLANET INTERACTIONS IN THE WASP-12 SYSTEM
in The Astrophysical Journal
Hennemann M
(2012)
The spine of the swan: a Herschel study of the DR21 ridge and filaments in Cygnus X
in Astronomy & Astrophysics
Description | This supported Astronomical Research at the Open University. Outputs have been reported in the Peer reviewed and unrefereed literature |
Exploitation Route | The results and outputs have informed the following Consolidated grant, into which this was rolled. |
Sectors | Education |
Description | Some of the research was used on TV news programmes. |
Sector | Education |
Impact Types | Societal |