'Mass function' diaporamas de présentation

Observing Black Holes With 1m-Class Telescopes

Observing Black Holes With 1m-Class Telescopes. Charles Bailyn Yale University.

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What IGM knows about the star-formation... An X-ray perspective.

What IGM knows about the star-formation... An X-ray perspective. Bookkeeping of energy and metal ejection IMF+AGN-cooling Tracing the LSS Role of clusters in the chemical evolution of the Universe. A. Finoguenov (MPE). Studying the Cosmic Galaxy and Star Formation History. Protocluster

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Current and Future Constraints on Models of Cosmic Acceleration

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Weighing in on Neutron Stars

Weighing in on Neutron Stars. Varun Bhalerao California Institute of Technology. Collaborators: F. Harrison, S. Kulkarni , Marten van Kerkwijk , and others. Weighing in on Neutron Stars. Why?. How?. What?. Classes of objects Examples Upcoming results. Varun Bhalerao.

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An upper limit to the masses of stars

An upper limit to the masses of stars. Donald F. Figer STScI Collaborators: Sungsoo Kim (KHU) Paco Najarro (CSIC) Rolf Kudritzki (UH) Mark Morris (UCLA) Mike Rich (UCLA). Arches Cluster Illustration. Outline. Introduction to the problem Observations Analysis Violators? Conclusions.

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630 views • 43 slides

???-2007, ??????, 17-22 ???????? 2007

???-2007, ??????, 17-22 ???????? 2007. Jets activity from RATAN and X-ray monitoring of microquasars Sergei Trushkin, N. Bursov, N. Nizhelskij SAO RAS T. Kotani, N. Kawai, M.Tsuboi ( Tokyo Tech, NRO ) ?. RATAN-600 radio telescope. North Caucas, al:1000 m band: 1-30 Ghz, 5-30mJy

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Cosmological growth of supermassive black holes: a synthesis model for accretion and feedback

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The Theory/Observation connection lecture 3 the (non-linear) growth of structure

The Theory/Observation connection lecture 3 the (non-linear) growth of structure. Will Percival The University of Portsmouth. Lecture outline. Spherical collapse standard model dark energy Virialisation Press-Schechter theory the mass function halo creation rate

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Phase Transitions of Strong Interaction System in Dyson-Schwinger Equation Approach

Phase Transitions of Strong Interaction System in Dyson-Schwinger Equation Approach. Yu-xin Liu ????? Department of Physics, Peking University, China. Outline I. Introduction II. The Approach

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Discrete Random Events

Discrete Random Events. Thurs. March 11, 1999 Review with Examples Discrete Outcome Sample Spaces Influence Diagrams & Probability Trees Moments (e.g., expectation, variance, kth central) Probability Functions (Marginal, Joint, Conditional)

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Gravitational radiation from Massive Black Hole Binaries

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An upper limit on the spin in GX 339-4

An upper limit on the spin in GX 339-4. Mari Kolehmainen & Chris Done Durham University. Determining the BH spin. Currently two methods shape of the Fe line from reflected emission continuum fitting of disc dominated spectra GX 339-4 widely studied in terms of Fe line

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Impact of Early Dark Energy on non-linear structure formation

Impact of Early Dark Energy on non-linear structure formation. Margherita Grossi MPA, Garching Advisor : Volker Springel. 3rd Biennial Leopoldina Conference on Dark Energy LMU Munich, 10 October 2008. Early dark energy models.

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Dense cores in the W3 GMC

Dense cores in the W3 GMC. Toby Moore James Allsopp Liverpool John Moores University UK. 850 um continuum. 850 um continuum. 850- ? m clumps in the W3 GMC. 319 dense clumps found above the noise contamination limit ( 280mJy ? 13 M ? )

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Kylie Minogue Asset Models & Who cares anyway

Kylie Minogue Asset Models & Who cares anyway . Martyn Dorey Consultant. 2 December 2003.

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The low-mass part of the IMF From solar neighborhood to galactic implications

The low-mass part of the IMF From solar neighborhood to galactic implications. Mass-magnitude relations The Luminosity Function ? The Mass Function The Substellar regime The galactic implication : M/L ratio. Gilles CHABRIER C.R.A.L., ENS-Lyon. Mass-Magnitude relationships.

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Edo Berger Harvard University

The Host Galaxies of High-Redshift GRBs. Edo Berger Harvard University. Outline. 1. GRBs at z<1: Is there a low-metallicity bias?. 2. The ISM of high-redshift galaxies. 3. DLA counterparts & the M-Z relation at z>2. Spitzer stack. Long GRBs Hosts: Metallicity?. metallicity.

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Nearby Galaxies on GMC Scales:

Nearby Galaxies on GMC Scales:. Massive complexes, cold dust, and the effect of environment Christine Wilson McMaster University. Interferometric Surveys for GMCs in Nearby Galaxies 1990-2000. Spiral Galaxies: M33: 44 clouds (Wilson & Scoville 1990, 1992, Viallefond et al. 1992)

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Dynamical Evolution and the Mass Function of Globular Cluster Systems

Dynamical Evolution and the Mass Function of Globular Cluster Systems. Steve Zepf and Enrico Vesperini Chris Waters Keith Ashman Arunav Kundu.

171 views • 7 slides