Open University Rolling Grant 2009 - 2014
Lead Research Organisation:
The Open University
Department Name: Physical Sciences
Abstract
The OU Astronomy Group seeks continuation of its Rolling Grant to support a program of observational, theoretical, laboratory and space based astronomical research and instrumentation development. Theme 1 Star formation: This theme aims to understand star formation of our Galaxy and the local universe, focussing on near and far infrared studies. We will pursue four interlinked projects working within our access to the Guaranteed Time data from the AKARI space infrared telescope, the LOFAR radio telescope, and ESO facilities. The projects lie at the heart of star formation astrophysics, building on past work on molecular cloud structure, far-IR astronomy and triggered and high mass star formation. Project 1.1 ASTRO-F Galactic Plane Survey Project 1.2 Massive star and starburst cluster formation Project 1.3 HERSCHEL Survey exploitation Project 1.4 LOFAR Galactic Plane Survey Theme 2 Planetary Astrophysics: This area includes observational searches for Exoplanets; exoplanet characterisation with HST and Spitzer, modelling Exoplanet atmospheres; the interior structure of Exoplanets; and the dynamics and migration physics involved in various planetary architectures; and models and exploitation of data from solar system terrestrial planetary atmospheres. Project 2.1 Exoplanet Dynamics Project 2.2 Exoplanet Structure and Evolution Project 2.3 Solar System terrestrial planetary atmospheres Theme 3 Extragalactic Infrared astronomy & Cosmology: This is an integrated research programme to trace the cosmic evolution of star-forming galaxies using major international far-infrared and submm-wave legacy surveys / key projects. Project 3.1 SCUBA-2 and AKARI Legacy Surveys Project 3.2 The HERSCHEL ATLAS Key Project Project 3.3 The Cosmic Near-Infrared Background Theme 4 Extreme Environment astrophysics: This program explores the interrelation between galactic environment and relativistic object content in nearby galaxies, to provide insights into high-mass star formation, relativistic object formation and high-energy phenomena that cannot be gained from observations in our own Galaxy alone; to study the counterparts of high-energy sources we identify in our X-ray surveys of nearby galaxies; and conduct numerical simulations to model the nature of the accretion flows and the nature of their X-ray populations Project 4.1 Relativistic accretors in nearby galaxies Project 4.2 Characterising compact accreting systems Project 4.3 Magnetic Cataclysmic Variable Populations Theme 5 Laboratory Astrochemistry; Exploring Chemical Complexity: The research is targeted at simulating chemical and physical processes within star and planet formation regions and planetary atmospheres and surfaces; The research programme is focused on two projects (i) exploring the nature of chemical complexity in the ISM and (ii) identification of biomarkers that will be used to exploit extant data, and lead to the identification of robust biogenic biomarker signals in Exoplanet atmospheres and surfaces. Project 5.1 The Chemistry of Star and Planet Formation. Project 5.2 Identifying biosignatures for Exoplanetary studies; Theme 6 Astronomical Instrumentation Development for Space Missions: This proposal aims to promote radiation damage studies for future space missions which are within the STFC programme. The activity includes: a) Laboratory study of radiation damage and other environmental factors affecting scientific instrumentation on space missions, b) To provide low-level support to our collaboration with China on their first national X-ray astronomy mission, HXMT, c) To provide support at the early stage of future project studies, for both space and ground based instrumentation Project 6.1 Laboratory Studies of Radiation Damage (1 PDRA) Project 6.2 Radiation Damage support for the HXMT project
Publications
Negueruela I
(2010)
Another cluster of red supergiants close to RSGC1
in Astronomy and Astrophysics
Nguyên Luong Q
(2011)
The Herschel view of massive star formation in G035.39-00.33: dense and cold filament of W48 undergoing a mini-starburst
in Astronomy & Astrophysics
Nilsson R
(2010)
Kuiper belts around nearby stars
in Astronomy and Astrophysics
Norton A
(2012)
Time-Domain Astrophysics with SuperWASP
in Proceedings of the International Astronomical Union
Norton A
(2011)
Short period eclipsing binary candidates identified using SuperWASP
in Astronomy & Astrophysics
Omont A
(2013)
H 2 O emission in high- z ultra-luminous infrared galaxies
in Astronomy & Astrophysics
Omont A
(2011)
Observation of H 2 O in a strongly lensed Herschel -ATLAS source at z = 2.3
in Astronomy & Astrophysics
Oonk J
(2014)
Discovery of carbon radio recombination lines in absorption towards Cygnus A
in Monthly Notices of the Royal Astronomical Society
Oyabu S
(2010)
AKARI infrared bright source catalogues
Palmeirim P
(2013)
Herschel view of the Taurus B211/3 filament and striations: evidence of filamentary growth?
in Astronomy & Astrophysics
Parsons H
(2012)
Molecular clumps in the W51 giant molecular cloud Molecular clumps in W51
in Monthly Notices of the Royal Astronomical Society
Paunzen E
(2010)
A photometric long-term study of chemically peculiar stars in open clusters
in Astronomy & Astrophysics
Paunzen E
(2013)
A photometric study of chemically peculiar stars with the STEREO satellites - II. Non-magnetic chemically peculiar stars?
in Monthly Notices of the Royal Astronomical Society
Pearson C
(2014)
The First Source Counts at 18 microns from the AKARI NEP Survey
Pearson C
(2010)
The AKARI FU-HYU galaxy evolution program: first results from the GOODS-N field
in Astronomy and Astrophysics
Pearson C
(2014)
The first source counts at 18 µm from the AKARI NEP Survey
in Monthly Notices of the Royal Astronomical Society
Pearson C
(2010)
Source counts at 15 microns from the AKARI NEP survey
in Astronomy and Astrophysics
Pearson C
(2012)
THE SYNERGY OF LARGE AREA SURVEYS WITH AKARI AND HERSCHEL
in Publications of The Korean Astronomical Society
Peretto N
(2012)
The Pipe Nebula as seen with Herschel : formation of filamentary structures by large-scale compression?
in Astronomy & Astrophysics
Petrosyan A
(2011)
THE MARTIAN ATMOSPHERIC BOUNDARY LAYER
in Reviews of Geophysics
Pezzuto S
(2012)
Herschel observations of B1-bS and B1-bN: two first hydrostatic core candidates in the Perseus star-forming cloud
in Astronomy & Astrophysics
Pinte C
(2010)
The Herschel view of GAS in Protoplanetary Systems (GASPS) First comparisons with a large grid of models
in Astronomy and Astrophysics
Podio L
(2012)
Herschel /PACS observations of young sources in Taurus: the far-infrared counterpart of optical jets
in Astronomy & Astrophysics
Polehampton E
(2010)
The ISO Long Wavelength Spectrometer line spectrum of VY Canis Majoris and other oxygen-rich evolved stars
in Astronomy and Astrophysics
Polychroni D
(2013)
TWO MASS DISTRIBUTIONS IN THE L 1641 MOLECULAR CLOUDS: THE HERSCHEL CONNECTION OF DENSE CORES AND FILAMENTS IN ORION A
in The Astrophysical Journal
Description | This supported a varied programme of astronomical research at the Open University. Outputs have been published in peer-reviewed, and unrefereed papers and catalogues. |
Exploitation Route | These results were rolled into the next Consolidated Grant that was awarded. |
Sectors | Education |
Description | As a basis for a number of Television News interviews on different astronomical subjects As part of Open University Teaching material |
First Year Of Impact | 2009 |
Sector | Education |
Impact Types | Societal |
Description | Edinburgh |
Organisation | University of Edinburgh |
Department | Theoretical Particle Physics (PPT) Research Group |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Contribution of expertise; also some travel funds for visits of the collaborator to Durham and Glasgow. |
Collaborator Contribution | A member of Edinburgh University joined an existing project looking at properties of soft gluons in multiparton scattering. This has led to new developments, aided by the combination of complementary expertise. Edinburgh have also contributed with some financial assistance (e.g. accommodation for visits). |
Impact | So far there have been two published research papers (see publications). |
Start Year | 2010 |