Road Map to DARWIN and Beyond: a Ten Year Strategy for Exoplanet Research in the UK 2006 - 2015
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VISTA Variables in the Via Lactea (VVV)
What is the structure of the inner bulge? How did the MW form? VVV is a proposed public survey to be VISTA Variables in the Via carried out with VISTA at Paranal Observatory between 2007 and 2011. It will map repeatedly the entire Milky Way Lactea (VVV) bulge, as well as the inner southern disk, covering a total area of about 600 sq deg containing 5x108 point sources, 40 known globular clusters and more than one hundred known open clusters. The main survey products will be a JHK atlas of the MW bulge and inner disk, and RRab δSct (Cepheids) catalogues of variable point sources and RRc high proper-motion objects. The multi- SRs N epoch photometry will allow the E identification and phasing of periodic variable stars, as well as microlensing events and planetary transits. We plan to Figure 3. MACHO pulsating variables in the unveil the 3-D structure of the inner bulge direction of the MW bulge (Alcock et al. 1998). and disk of the MW using well understood Å 2MASS Magnitude, color, period and amplitude information allow reliable classification of distance indicators such as RR Lyrae variable stars. stars and clump giants. The survey will Å 1 epoch also detect tens of star formation regions Å all and allow to test the environmental dependence of star formation. The VISTA observations will be combined with data Figure 1. JH and JK color-magnitude Figure 2. JK photometric errors diagrams of a crowded bulge field expected in bulge crowded fields from MACHO, OGLE, EROS, 2MASS, obtained with NTT+ SOFI (Zoccali et al. -
The New Astrometry Frontier Proposal for a Medium Size Mission Opportunity in ESA’S Science Programme (M5) Mission
THEIA Microarcsecond Astrometric Observatory Graphisme : Roxane Arleo Roxane : Graphisme Faint objects in motion : the new astrometry frontier Proposal for a medium size mission opportunity in ESA’s science programme (M5) mission Theia lead proposer : Prof Céline Bœhm Theia Contact information Theia: Faint objects in motion. The new astrometry frontier. Theia’s Lead proposer: Prof Céline Bœhm, Physics Department, Durham University, DH1 3LE Durham, UK, tel: +44 (0)191 334 3747, email: [email protected] Availability to support the study activities : 80 % National contact points UK C. Boehm G. Anglada-Escudé [email protected] [email protected] PT A. Krone-Martins A. Amorim [email protected] [email protected] FR G. Mamon F. Malbet [email protected] [email protected] IT A. Sozzetti R. Claudi [email protected] [email protected] CH F. Courbin B. Holl frederic.courbin@epfl.ch [email protected] ES E. Villaver X. Luri [email protected] [email protected] SE K. Freese D. Spolyar [email protected] [email protected] DE L. Labadie A. Quirrenbach [email protected] [email protected] USA M. Shao B. McArthur [email protected] [email protected] with the contribution of AMDL Space (A.M. DiLellis), Aurora Technology BV (A. Mora), CNES (J.M. Le Duigou), DAPCOM Data Services S.L. (J. Portell), e2v (J. Hopgood, J.-F. Bruyeres-Inza, D. Morris), Thales Alenia Space (J.P. Prost, P. -
THE STAR FORMATION NEWSLETTER an Electronic Publication Dedicated to Early Stellar Evolution and Molecular Clouds
THE STAR FORMATION NEWSLETTER An electronic publication dedicated to early stellar evolution and molecular clouds No. 137 — 9 March 2004 Editor: Bo Reipurth ([email protected]) Abstracts of recently accepted papers A Single Circumstellar Disk in the SVS 13 Close Binary System Guillem Anglada1, Luis F. Rodr´ıguez2, Mayra Osorio1, Jos´eM. Torrelles3, Robert Estalella4, Maria T. Beltr´an5 and Paul T. P. Ho6 1 Instituto de Astrof´ısicade Andaluc´ıa,CSIC, Camino Bajo de Hu´etor 24, E-18008 Granada, Spain 2 Centro de Radioastronom´ıa y Astrof´ısica, UNAM, Apartado Postal 3-72 (Xangari), 58090 Morelia, Michoac´an, M´exico 3 Instituto de Ciencias del Espacio (CSIC)-IEEC, Gran Capit`a,2, 08034 Barcelona, Spain 4 Departament d’Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal 647, E-08028 Barcelona, Spain 5 Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy 6 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA E-mail contact: [email protected] We present Very Large Array observations at 7 mm of the sources IRAS 2A, IRAS 2B, MMS2, MMS3 and SVS 13, in the NGC1333 region. SVS 13 is a young close binary system whose components are separated by 65 AU in projection. Our high angular resolution observations reveal that only one of the components of the SVS 13 system (VLA 4B) is associated with detectable circumstellar dust emission. This result is in contrast with the well known case of L1551 IRS5, a binary system of two protostars separated by 45 AU, where each component is associated with a disk of dust. -
Future Science Prospects for AMI
Future Science Prospects for AMI Keith Grainge,1, 2 Paul Alexander,1, 2 Richard Battye,3 Mark Birkinshaw,4 Andrew Blain,5 Malcolm Bremer,4 Sarah Bridle,6 Michael Brown,3 Richard Davis,3 Clive Dickinson,3 Alastair Edge,7 George Efstathiou,2 Robert Fender,8 Martin Hardcastle,9 Jennifer Hatchell,10 Michael Hobson,1 Matthew Jarvis,11, 12 Benjamin Maughan,4 Ian McHardy,8 Matthew Middleton,7 Anthony Lasenby,1, 2 Richard Saunders,1, 2 Giorgio Savini,13 Anna Scaife,8 Graham Smith,14 Mark Thompson,9 Glenn White,15, 16 Kris Zarb-Adami,11, 17 James Allison,18 Jane Buckle,1 Alberto Castro-Tirado,19 Maria Chernyakova,20 Roger Deane,21 Farhan Feroz,1 Ricardo G´enova-Santos,22 David Green,1 Diana Hannikainen,23, 24 Ian Heywood,11 Natasha Hurley-Walker,25 R¨udigerKneissl,26, 27 Karri Koljonen,24 Shrinivas Kulkarni,28 Sera Markoff,29 Carrie MacTavish,2 Michael McCollough,30 Simone Migliari,31 Jon M. Miller,32 James Miller-Jones,25 Malak Olamaie,1 Zsolt Paragi,33 Timothy Pearson,34 Guy Pooley,1 Katja Pottschmidt,35 Rafael Rebolo,22 John Richer,1 Julia Riley,1 J´er^omeRodriguez,36 Carmen Rodr´ıguez-Gonz´alvez,37 Anthony Rushton,38 Petri Savolainen,24 Paul Scott,1 Timothy Shimwell,39 Marco Tavani,40 John Tomsick,41 Valeriu Tudose,42 Kurt van der Heyden,21 Alexander van der Horst,43 Angelo Varlotta,44 Elizabeth Waldram,1 Joern Wilms,45 Andrzej Zdziarski,46 Jonathan Zwart,12 Yvette Perrott,1 Clare Rumsey,1 and Michel Schammel1 1Astrophysics Group, Cavendish Laboratory, J J Thomson Avenue, Cambridge, CB3 0HE UK 2Kavli Institute for Cosmology Cambridge, Madingley