Preliminary modelling with CLOUDY. What is still to do ? Abundance analysis, Velocity field analysis, Archival IR data can be included for StWr 2-21. Project status : ...
Dynamics, abundances with Mark Wilkinson, Rosie Wyse, ... dispersion profile, with assumed isotropy, and smooth functional fit to the light profile ...
Mass to light ratios vs. Galaxy absolute V magnitude (Gilmore et al. 2006) ... Carigi, Hernandez & Gilmore (2002) computed models for 4 dSphs by assuming SF ...
dIrrs and BCDs tend to have gasping' rather *than bursting' SF. Most dEs and dSphs have young and ... Each galaxy is individual - there is no one size fits all' ...
Along with Sagittarius , it is the only dSph known to host globular clusters. ... possess mean characteristics intermediate between the two Oosterhoff groups ...
Mei-Yin Chou (UVa - Ph.D. thesis), Katia Cunha, ... Testing the connection to the Monoceros stream. ... Tri-And Star Cloud not chemically linked to Monoceros. ...
New detailed star formation histories of all classic Local Group dwarfs ... Primordial gas does not cool efficiently in halos with T 104 K but we may also ...
Open Questions in Dwarf Galaxy Formation. Is the 'missing satellites problem' still a problem? (can we reproduce dwarf galaxy numbers and spatial distribution? ...
Steve Majewski (UVa), Katia Cunha, Verne Smith (NOAO), David Mart nez-Delgado (IAC) ... Sgr core of today differs from Sgr core of 'yester- gigayears' ...
Fabry-Perot spectrographs and IFU: velocity information for the whole field, but ... systems: velocity dispersion. Rotationally-supported systems: rotation ...
Chemo-dynamique des populations stellaires de la Galaxie (disques, halo, r gions internes) ... assemblage de halo ? Evolution propre de ces syst mes ...
You see a Dark Apple, I see Non-Newtonian Field HongSheng Zhao @St Andrews, SUPA This is NOT an Apple (Magritte) Let s call the whole thing Potato-Tomato ...
... variables in the isolated dwarf galaxies Tucana & LGS3. Edouard Bernard ... Not affected by gravitationally dominant galaxies, the Milky Way & M31 (Kravtsov ...
Evan Kirby (Santa Cruz) Or, Why Segue 1 Is Not a Star Cluster. Galaxy formation ... Dwarf galaxies are the closest and densest dark matter-dominated objects ...
`The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems' ... Lick Indices: Breaking Age/Metallicity Degeneracy. Age-s correlation? ...
Some observed properties of Dark Matter: Gerry Gilmore. Institute ... dispersion profile, with assumed isotropy, and smooth functional fit to the light profile ...
Outline Background to the register Where we are now First phase of registration Next ... for setting up the Register Jenny Griffiths project manager Launched ...
100 for Leo I. Wide exploration of parameter space: Mass: 1 x 106 ... Very little stripping can cause flat/rising velocity dispersion profile. Result for Leo I ...
Title: LDP 2005-08 Implications for Public Health Information Author: MilliganJ Last modified by: MilliganJ Created Date: 1/10/2005 1:50:11 PM Document presentation ...
The Role of the DPH and Joint Strategic Needs Assessment George Leahy Head of Public Health Development Department of Health Purpose To discuss the new Commissioning ...
National Astronomical Observatories, Chinese Academy of Science. Background ... Precise measurements of basic quantities for individual stars are possible for ...
Dr. Ashok P. Shroff, MD, Dr. Hardik A. Shroff, MD. Dr. Dishita H. Shroff, MD, Dr. V. D. ... Complicated aphakia. BCVA: HM only. IOP: 17 mmHg. Treatment Attempted ...
Concerns of commentators prior to study (e.g. HS Committee) Too many onerous national targets ... analysis of free text comments. Results. 1.Return Rate ...
soft merging ( la Sagittarius dwarf) ... dynamical equilibrium: a suitable scenario to ... role of DM halos: self-regulated evolution; exponential profiles ...
Environments ranging from field to Virgo Cluster-like density (core of the Coma I group) ... fundamentally new things extending to the 10Mpc groups and Virgo? ...
Rotation curves of spirals can be explained with MOdified Newtonian Dynamics ... Classical field theory (modified Poisson equation) Bekenstein & Milgrom (1984) ...
Is the outer halo filled with tidal streams from disrupted dwarf galaxies that ... (Bullock et al. 2002, Font et al. 2001, 2005, Johnston et al. 2002, etc. ...
Extremely low internal accelerations make them the perfect testing ground for ... where b measures the anisotropy in the velocity distribution, n is the 3-D ...
Mixed Perceptions on ADPH and its role/function. Fit between ... Robert Burns, Poem 'To a Louse' - verse 8. Scottish national poet (1759 - 1796) www.adph.org.uk ...
Presentamos resultados preliminares de un estudio espectrofotom trico de la ... del Grupo de NGC5044, sus magnitudes absolutas ser an anormalmente d biles (Mg -14) ...
Healthy People, Healthy Lives Our strategy for public health in England The Health Background Britain has amongst the worst levels of obesity in the world.
Healthy Lives, Healthy People Our strategy for public health in England Funding and commissioning routes Lucinda Cawley Consultant in Public Health | Associate ...
Making it Happen. Evidence and information. Workforce capacity and capability ... Political will and commitment. Power and advocacy. Confronting wicked problems' ...
... NFW profile from Taylor & Babul, 2004, 2005 ... Milky Way Halo simulated by Taylor & Babul (2005) All-sky map of DM gamma ray emission (Baltz 2006) ...