Gas, dust and stars: the life cycle of galaxies
Lead Research Organisation:
University of Manchester
Department Name: Physics and Astronomy
Abstract
The Universe is in constant evolution. Stars form out of clouds of gas. They live by burning hydrogen into helium, and later into carbon and oxygen. The nuclear burning takes place in the centre of the stars, but the products are brought to the surface and change the composition of the star. At the end of its life, the star will expel half or more of its mass in a catastrophic wind. The material blown off from these evolved stars forms fantastic and beautiful structures (e.g. Planetary Nebulae), we don't fully understand the physics that generates the structures but suspect that binary systems and magnetic fields are a factor. The wind expels the newly formed elements into space where they enrich clouds of gas. Thus, the next generation of stars will benefit from these new elements. At the same time, some elements condense as small particles, forming dust grains. These grains are also added to the clouds. When new stars form from this cloud, some of this dust will start the formation of planets. We are studying this cycle of evolution of stars, dust and gas. We study the input of new dust into the interstellar medium, looking at a variety of objects, with special emphasis on conditions of low metallicity, as existed in the early Universe. We study how stars form, especially stars more massive than the Sun. We look at the properties of dust over a complete galaxy (the Large Magelanic Cloud is the main target). We also study the chemistry of interstellar and circumstellar gas. We are also trying to understand how the presence of binary systems can affect the physics of the mass-loss process. The solar system is itself the result of this Universe of evolution. Dust left over from its formation is still present, incorporated in large grains or even comets and meteorites. Space craft are now collecting this dust. One of the goals of our research is to find the progeny of the proto-solar dust, among the outflows of other stars.
Publications
De Vries B
(2010)
Determining the forsterite abundance of the dust around asymptotic giant branch stars
in Astronomy and Astrophysics
Lagadec E
(2010)
The low wind expansion velocity of metal-poor carbon stars in the Halo and the Sagittarius stream
in Monthly Notices of the Royal Astronomical Society
Hounsell R
(2010)
EXQUISITE NOVA LIGHT CURVES FROM THE SOLAR MASS EJECTION IMAGER (SMEI)
in The Astrophysical Journal
Duarte-Cabral A
(2010)
The physical and dynamical structure of Serpens Two very different sub-(proto)clusters
in Astronomy and Astrophysics
Srinivasan S
(2010)
The mass-loss return from evolved stars to the Large Magellanic Cloud III. Dust properties for carbon-rich asymptotic giant branch stars
in Astronomy & Astrophysics
Tideswell D
(2010)
The abundance of HNCO and its use as a diagnostic of environment
in Astronomy and Astrophysics
Sloan G
(2010)
SPITZER SPECTROSCOPY OF MASS-LOSS AND DUST PRODUCTION BY EVOLVED STARS IN GLOBULAR CLUSTERS
in The Astrophysical Journal
De Beck E
(2010)
Probing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles II. CO line survey of evolved stars: derivation of mass-loss rate formulae
in Astronomy & Astrophysics
Davis C
(2010)
The JCMT Legacy Survey of the Gould Belt: a first look at Taurus with HARP
in Monthly Notices of the Royal Astronomical Society
Ellingsen S
(2010)
Masers associated with high-mass star formation regions in the Large Magellanic Cloud Masers in the LMC
in Monthly Notices of the Royal Astronomical Society
Gielen C
(2010)
SPITZER-IRS spectral fitting of discs around binary post-AGB stars ( Corrigendum )
in Astronomy and Astrophysics
Caswell J
(2010)
The 6-GHz methanol multibeam maser catalogue - I. Galactic Centre region, longitudes 345° to 6° Methanol maser catalogue: Galactic Centre
in Monthly Notices of the Royal Astronomical Society
Hony S
(2010)
The Herschel revolution: Unveiling the morphology of the high-mass star-formation sites N44 and N63 in the LMC
in Astronomy and Astrophysics
Van Der Wiel M
(2010)
Chemical stratification in the Orion Bar: JCMT spectral legacy survey observations (Corrigendum)
in Astronomy and Astrophysics
Otsuka M
(2010)
Dust in the bright supernova remnant N49 in the LMC
in Astronomy and Astrophysics
Roberts H
(2010)
Dense molecular gas towards W49A: a template for extragalactic starbursts?
in Astronomy & Astrophysics
Cami J
(2010)
SPECTRAFACTORY.NET: A DATABASE OF MOLECULAR MODEL SPECTRA
in The Astrophysical Journal Supplement Series
Rodríguez-Gil P
(2010)
The orbital period of V458 Vulpeculae, a post-double common-envelope nova
in Monthly Notices of the Royal Astronomical Society: Letters
Graves S
(2010)
The JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARP GBS: first look at Serpens
in Monthly Notices of the Royal Astronomical Society
Gesicki K
(2010)
Disk evaporation in a planetary nebula
in Astronomy and Astrophysics
Jones D
(2010)
Abell 41: shaping of a planetary nebula by a binary central star? Abell 41: shaped by a binary central star
in Monthly Notices of the Royal Astronomical Society
Peretto N
(2010)
Mapping the column density and dust temperature structure of IRDCs with Herschel
in Astronomy and Astrophysics
McDonald I
(2010)
RUSTY OLD STARS: A SOURCE OF THE MISSING INTERSTELLAR IRON?
in The Astrophysical Journal
Smolders K
(2010)
When an old star smolders On the detection of hydrocarbon emission from S-type AGB stars
in Astronomy and Astrophysics
Buckle J
(2010)
The JCMT Legacy Survey of the Gould Belt: a first look at Orion B with HARP
in Monthly Notices of the Royal Astronomical Society
Gordon K
(2010)
Determining dust temperatures and masses in the Herschel era: The importance of observations longward of 200 micron
in Astronomy and Astrophysics
Sale S
(2010)
The structure of the outer Galactic disc as revealed by IPHAS early A stars
in Monthly Notices of the Royal Astronomical Society
{Molster}, F.~J. And {Waters}, L.~B.~F.~M. And {Kemper}, F.
(2010)
The Mineralogy of Interstellar and Circumstellar Dust in Galaxies
Meixner M
(2010)
HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE): The Large Magellanic Cloud dust
in Astronomy and Astrophysics
Green J
(2010)
The 6-GHz methanol multibeam maser catalogue - II. Galactic longitudes 6° to 20° Methanol maser catalogue: 6° to 20°
in Monthly Notices of the Royal Astronomical Society
Boyer M
(2010)
Cold dust in three massive evolved stars in the LMC
in Astronomy and Astrophysics
Peretto N
(2010)
A STATISTICAL STUDY OF THE MASS AND DENSITY STRUCTURE OF INFRARED DARK CLOUDS
in The Astrophysical Journal
Sargent B
(2010)
THE MASS-LOSS RETURN FROM EVOLVED STARS TO THE LARGE MAGELLANIC CLOUD. II. DUST PROPERTIES FOR OXYGEN-RICH ASYMPTOTIC GIANT BRANCH STARS
in The Astrophysical Journal
Giammanco C
(2010)
IPHAS extinction distances to planetary nebulae
in Astronomy & Astrophysics
Molinari S.
(2010)
Hi-GAL: The Herschel Infrared Galactic Plane Survey
in PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
Kemper F.
(2010)
The SAGE-Spec Spitzer Legacy Program: The Life Cycle of Dust and Gas in the Large Magellanic Cloud
in PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
Van Loon J
(2010)
A SPITZER SPACE TELESCOPE FAR-INFRARED SPECTRAL ATLAS OF COMPACT SOURCES IN THE MAGELLANIC CLOUDS. I. THE LARGE MAGELLANIC CLOUD
in The Astronomical Journal
Hajduk M
(2010)
Binary [WR] and wels central stars of planetary nebulae Binary WR and wels central stars of PNe
in Monthly Notices of the Royal Astronomical Society
Jones D
(2010)
Kinematics of the ring-like nebula SuWt 2
in Monthly Notices of the Royal Astronomical Society
Asanok K
(2010)
OH and H 2 O masers towards the star-forming region S140-IRS1
in Monthly Notices of the Royal Astronomical Society
Molinari S
(2010)
Clouds, filaments, and protostars: The Herschel Hi-GAL Milky Way
in Astronomy and Astrophysics
Minniti D.
(2011)
The VVV Survey of the Milky Way: first year results
in Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
Lykou F
(2011)
A disc inside the bipolar planetary nebula M2-9
in Astronomy & Astrophysics
Sloan G
(2011)
THE IDENTIFICATION OF PROBABLE SiS EMISSION AT 13-14 µm IN SPECTRA OF GALACTIC S STARS
in The Astrophysical Journal
Van Breemen J
(2011)
The 9.7 and 18 µ m silicate absorption profiles towards diffuse and molecular cloud lines-of-sight
in Astronomy & Astrophysics
Woods P
(2011)
The SAGE-Spec Spitzer Legacy programme: the life-cycle of dust and gas in the Large Magellanic Cloud - Point source classification I SAGE-Spec - Point source classification I
in Monthly Notices of the Royal Astronomical Society
Osborne J
(2011)
THE SUPERSOFT X-RAY PHASE OF NOVA RS OPHIUCHI 2006
in The Astrophysical Journal
Wilcock L
(2011)
The initial conditions of high-mass star formation: radiative transfer models of IRDCs seen in the Herschel Hi-GAL survey
in Astronomy & Astrophysics
Oliveira J
(2011)
Ice chemistry in massive young stellar objects: the role of metallicity Ice chemistry in massive young stellar objects
in Monthly Notices of the Royal Astronomical Society: Letters
Sabin L
(2013)
New Candidate Planetary Nebulae in the IPHAS Survey: the Case of Planetary Nebulae with ISM interaction
in Publications of the Astronomical Society of Australia
Description | The research covered a number of topics. A prime goal was to complete survey the Galaxy for sites of star formation and for evolved stars, using radio, sub-millimetre, infrared and optical surveys wavelengths. Much progress was made on this project, which will last over a decade. We also surveyed the Large Magellanic Clouds at wavelengths sensitive to dust .Sites of high-mass-star formation in the Galaxy were studied, later leading to a high impact program with the ALMA observatory. We worked on the catastrophic mass loss which ends the life of normal (sun-like) stars. and studied how this depends on the type of star. |
Exploitation Route | This is continuing research, widely disseminated through papers and meetings, and leading to follow-on grants and observing programs, both from the applicants and other teams in the world. |
Sectors | Education |
Description | The research covered in this award has featured heavy in our outreach activities. The study of planetary nebulae especialy is visually very appealing. During this grant, outreach activities at the JBCA operated through the Visitor Centre at the Observatory, the JBCA website, working with schools and community groups, and strong links with both the print and broadcast media. The strength of the outreach programme was recognised by the award of grants from STFC, the IoP, the Royal Academy of Engineering, the Arts Council and Agilent Technologies. The Jodrell Bank Visitor Centre has exhibitions on astronomy and associated technology and attracted 70,000 visitors each year, around half of whom are school age. It is widely agreed that astronomy and space science/technology, symbolised by iconic facilities such as Jodrell Bank, draws young people into studying science and then into the wider economy (e.g. Barstow report Bringing space into school science, Oct 2005). The success lead to the acceptance by the University and Northwest development agency for an ambitious new centre at Jodrell Bank, to be a signature project for the northwest region, and the UK as a whole. The unique became a vital part of the bid for hosting the SKA International Office at the Observatory which later added 60 high level jobs to Cheshire East. JBCA also delivers innovative public engagement events, such as: First Light - live performance of a new composition featuring signals picked up live by the Lovell Telescope and from microphones placed on the structure itself, turning it into a giant musical instrument; Moonbounce - poems written for a national competition organised by The Times were recited in front of an audience and sent as radio signals to the Moon, their echoes were received 2.5 seconds later by the Lovell Telescope and played back live. The Jodrell website contains information for a wide range of audiences and receives around 140,000 visits each month. A highlight is The Jodcast, our podcast featuring astronomy news and in-depth interviews with scientists and engineers, now attracting over 2,000 downloads per twice-monthly episode. Jodrell has a 7-metre radio telescope with a digital hydrogen-line receiver which is controlled remotely over the web (http://www.jb.man.ac.uk/distance/observatory). This has been used for several years on undergraduate distance learning courses and has recently been piloted for use by schools in the UK and across Europe as part of the European Hands-On Universe project. |
First Year Of Impact | 2008 |
Sector | Education |
Impact Types | Cultural,Societal,Economic |
Description | Isabel Aleman |
Organisation | Universidade de São Paulo |
Country | Brazil |
Sector | Academic/University |
PI Contribution | Research facilities |
Collaborator Contribution | Salary and secondment of Isabel Aleman |
Impact | Research papers |
Start Year | 2009 |
Description | Phil Diamond |
Organisation | Commonwealth Scientific and Industrial Research Organisation |
Country | Australia |
Sector | Public |
PI Contribution | Secondment of Phil Diamond as a director of the institute |
Collaborator Contribution | Salary |
Impact | N/A |
Start Year | 2009 |
Description | Phil Diamond |
Organisation | Square Kilometre Array (SKA) Africa |
Country | South Africa |
Sector | Academic/University |
PI Contribution | Secondment of Phil Diamond as SKA director |
Collaborator Contribution | Salary |
Impact | N/A |
Start Year | 2012 |
Description | The Jodcast |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | Since 2006, we have produced a podcast called the Jodcast. This is led by our research students and reaches an audience of around 7,000 for each twice monthly show. The podcast includes the latest news in astronomy, interviews and ask an astronomer sections. Each month since Jan 2012 the show features a "Jodbite" in which one of the researchers in the group is interviewed about their work. Impact is measured by downloads: each episode gets about 5000 downloads. |
Year(s) Of Engagement Activity | 2006,2008,2009,2010,2011,2012,2013,2014,2015,2016 |
URL | http://www.jb.man.ac.uk/jodcast/ |