Astronomiska
Seminariet
i
Lund
Lundmarksalen i
Astronomihuset,
Sölvegatan 27
Tid: Normalt torsdagar
kl 14:15 (om inget annat anges)
Seminars at Lund
Observatory
Time: Normally on Thursdays, 14:15 (unless
stated otherwise)
VT 2010
January 11th, 2010, 14:15 (Monday! in Lundsmarksalen)
Bengt
Gustafsson, Instit. för
fysik, astronomi och rymdfysik, Uppsala University, Sweden
Is the Sun an oddball
-- and is that related to our existence?
January 21st,
2010, 14:15
Vivienne
Wild, Institut d'astrophysique de
Paris, France
Timing
the starburst AGN-connection
February 4th,
2010, 14:15
Karin Lind,
ESO,
Garching bei München, Germany
Observational
signatures
of
lithium
depletion
in
halo
stars
-
the
key to solving the cosmological lithium problem?
February 11th,
2010, 14:15
Sung Soo Kim,
Kyung Hee University, South
Korea
Star
Formation in the Central Molecular Zone
February 18th, 2010, 14:15
Daniel Malmberg, Lund Observatory, Sweden
The
effect of encounters on planetary systems in young stellar clusters
February 23rd,
2010, 15:30 (Tuesday at
3.30pm!, Physics
and
Astronomy
Colloquium in Sal B)
Antje Jackelén, Bishop of Lund, Sweden
What
Theology Can Do for Science
February 25th,
2010, 14:15
Sung-Chul Yoon, Argelander-Institut für Astronomie der
Universität Bonn, Germany
Evolution
of merging white dwarfs
February 26th, 2010, 10.30 (Friday at
10.30am!, in Lundmarksalen)
Hans Rickman, Instit. för
fysik, astronomi och rymdfysik, Uppsala University, Sweden
Delivery
of water to the early Earth
March
4th, 2010, 14:15
Mathias
Schultheis, Observatoire
de
Besancon,
France
Stellar populations
in the Galactic bulge
March
18th, 2010, 14:15
Susanne
Höfner, Department
of
Physics
&
Astronomy,
Uppsala
University,
Sweden
Starlight and
sandstorms: cool giants in high resolution
March 25th, 2010, 14:15
Pat Scott, Department of Physics,
Stockholm University, Sweden
The search for particle dark
matter
April 15th, 2010, 13:00 (Thursday at
1pm!, Physics and Astronomy Colloquium Sal B in Physics)
John Z. Larese, University of Tennessee, Knoxville, Oak Ridge
National Laboratory, USA
Neutrons, Nano-materials
and Molecular Adsorption
April 28th, 2010, 14:15
Joint Astronomy and
Theoretical Physics Seminar
Justin Read, University of Leicester, England
The
N-body problem in astronomy
Sandipan Mohanty,
Jülich Supercomputing
Center, Forschungszentrum, Jülich, Germany
The
N-body problems in computational biology
May 4th, 2010, 15:30 (Tuesday at
3.30pm!, Physics
and
Astronomy
Colloquium in Sal B)
Kajsa
Uvdal, Institutionen
för fysik, kemi och biologi, Linköping
University, Sweden
Nanoparticles
for
Biomedical
Imaging
May 6th, 2010, 14:15 (In Andromeda at 2.15)
Maura
McLaughlin, West Virginia
University, Department of Physics, USA
A Pulsar
Timing Array for Gravitational Wave Detection
May 10th-11th,
2010, Mon. 1.30-4pm, Tue. 9.30-12am (Monday and Tuesday, in Physics Sal B)
Gunnar
and
Gunnel Källén
Memorial
Symposium
on
"New
Horizons
in
Physics"
Monday
13.35
Ingolf
Lindau,
Stanford University, USA and Lund University, Sweden
The X-ray
free electron laser: a new and emerging research tool. Including first
results from the Linac Coherent Light Source (LCLS) at Stanford
Monday
15.00
Gérard
Mourou, Center
for Ultrafast Optical Science, University of Michigan, USA
New horizons with
ultra-high intensity lasers
Tuesday 09.30
Francis Halzen, Department of
Physics, University of Wisconsin, USA
Particle
astrophysics: closing in on the sources of cosmic rays
Tuesday 11.00
Brenda
Dingus, Los
Alamos National Laboratory, USA
The Latest High
Energy Observations of Gamma-Ray Bursts. Results from the GLAST/FERMI
space telescope
May 12th, 2010, 9-12 am (Wednesday morning in Lundmarksalen)
Ph.D. Seminars in
Astronomy,
Lund Observatory, Sweden
Astronomy and
Astrophysics students will present their ongoing thesis work
May 18th, 2010, 10:30 (Tuesday morning in Lundmarksalen)
Torgny
Karlsson, School
of
Physics,
The
University
of
Sydney, Australia
Uncovering the
chemical signatures of the first star clusters in the universe.
May 27th, 2010, (Lecture Hall
”Lundmarksalen”, Astronomy starting at 10.00 am.)
Faculty
of
Science,
Lund
University
Honorary
Doctors
of
Philosophy
2010
Prof.
Michael
Perryman, University
of
Heidelberg,
and
Max
Planck
Institute
for
Astronomy,
Heidelberg,
Germany
The Making of
History's Greatest Star Map
Prof. Peter Varga,
Surface
Physics Group, Vienna
University of Technology, Austria
Is an image worth more
than a 1000 words?
May 31st, 2010, 09.15 and
14:15
Master students final
presentations
Fredrik
Windmark, Lund
Observatory, Sweden
Astrophysical
validation of Gaia parallaxes
Carina Lagerholm, Lund
Observatory, Sweden
The Disk - Halo
Transition and the Search of Stellar Streams
June 1st, 2010, 10:15
Master students final
presentation
Nils
Håkansson, Lund
Observatory, Sweden
Horizontal
Adaptive Optics in the Ground Layer Atmosphere
June 1st, 2010, 14:15 (ESSS and Faculty of Science seminar in
Q 179, physics)
Gerhard
Grübel, Deutsches
Elektronen-Synchrotron (DESY), Hamburg, Germany
Femtosecond
magnetic X-ray scattering
June 1st, 2010, 15:30 (Joint Physics and Astronomy colloquium in Hall B, physics)
Eva
Olsson ,
Chalmers teknisk högskola, Department of Applied Physics, Sweden
Gripping the nanoworld - to see and manipulate on
the nanoscale
June 4th, 2010, 14:15
Master students final
presentations
Hannes Jensen, Lund Observatory,
Sweden
A Hundred Times Sharper Than Hubble:
Stellar Imaging With Intensity Interferometry
June 14th, 2010, 14:15 (Monday at
2.15pm!, in Lundmarksalen)
Fred
Adams, University of
Michigan, Department of Physics, USA
Dynamical Processes in
Extrasolar Planetary Systems
June 15th, 2010, 14:00 (Tuesday at
2pm!, Ph.D. Thesis defense in Lundmarksalen)
Daniel Malmberg, Lund Observatory, Sweden
The effect of
encounters on planetary systems in stellar clusters
June 16th, 2010, 10:00 (Wednesday at
10.00am! in Lundmarksalen)
Jack
Lissauer, Space Science
& Astrobiology Division, NASA Ames Research Center, USA
Exoplanets & Planet
Formation in the Kepler Era
June 17th, 2010, 14:15
Master students
final
presentations
Tobias
Albertsson, Lund Observatory,
Sweden
Collisions between
Jupiter-like planets
June 18th, 2010, 14:15
Markus Janson, Dept. of
Astronomy and Astrophysics, University of Toronto, Canada
Imaging
and
spectroscopy
of
extrasolar
planets
Seminars at Lund
Observatory
Time: Normally on Thursdays, 14:15 (unless
stated otherwise)
HT 2010
August
18th, 2010, 14:15 (Note: we will hold
the seminar on Wednesday at 2.15pm)
Benjamin
Knispel, Max
Planck
Institute
for
Gravitational
Physics,
IMPRS,
Germany
The Einstein@Home
Search for Arecibo's Tightest Binary Radio Pulsar
August
26th, 2010, 14:15
Jie Chen, Swedish Institute of
Space Physics, Lund, Sweden
Solar
coronal loops
September
2nd, 2010, 14:15
Jennifer Johnson, Department of
Astronomy, Ohio State University, USA
Nucleosynthesis in
the First Generations of AGB stars
September
7th, 2010, 15:00 (Joint Physics
& Astronomy Colloquium, Lecture hall, B physics)
Birger Schmitz, Department
of
Geology,
University
of Lund,
Sweden
Astrobiology
-
what
physicists
and
astronomers
should
know
about
dinosaurs
and
how
(almost)
everything is connected
September
9th, 2010, 13:45 (Note: we must
start
early at 1.45pm)
Ross
Church, Lund
Observatory, University of Lund, Sweden
Short gamma-ray bursts -- evidence for an
origin in globular clusters?
September
16th, 2010, 14:15
Mir
Abbas Jalali, Dept.
of
Mechanical
Engineering,
Sharif
University
of
Technology,
Iran
Finite Element
Modelling of Stellar Systems
September 23th, 2010, 14.15 (Note the seminar will be held in Cassiopeia)
Magister
thesis final presentation
Johan Ingjald,
Lund Observatory &
Örebro University, Sweden
Photon
Counting
in
Astronomy:
Evaluation
of
avalanche
photodiode
detectors
September
30th, 2010, 14.15
Richard Parker,
Institute
of
Astronomy,
ETH
Zurich,
Switzerland
Star and Planet
Formation: Constraints from Cluster Evolution
October
7th, 2010, 14:15
Robert Izzard, Argelander-Institut
für
Astronomie,
University
of
Bonn,
Germany
Fluid transfer between
binary stars
October
21st, 2010, 14:15
Martin
Pessah, Niels
Bohr
Institute,
Denmark
An Introduction to the Importance of
Magnetic Fields on Turbulent Angular Momentum Transport in Accretion
Disks
October
28th, 2010, 14:15
Helena Uthas,
School
of Physics and Astronomy, University of Southampton, UK
Observational Studies of
Cataclysmic Variables Evolution
November
2nd, 2010, 15:00 (Note: Tuesday
at 15:00 physics-astronomy colloquium)
Steven
Balbus, Laboratoire
de
Radioastronomie, École
Normale
Supérieure,
Paris,
France
Alpha Disks, the Magnetorotational
Instability, and Beyond
November 4th, 2010, 10:00
(Note: Thursday
morning
at 10:00am)
Steven
Balbus, Laboratoire
de
Radioastronomie, École
Normale
Supérieure,
Paris,
France
Probing the flywheels of Helios: what
makes the Sun go round
November
11th, 2010, 14.15
Alice
Quillen, Department
of
Physics
and
Astronomy,
University
of
Rochester,
USA
Dissecting the Milky Way disk and
halo: Clumps in tidal streams and in the disc velocity
distribution.
November
18th, 2010, 14.15
Thijs Kouwenhoven, Kavli Inst. for
Astronomy & Astrophysics, Peking University, China
The dynamical evolution of binary systems
and planetary systems in young star clusters
December 6th,
2010, 14:15 (Note: Monday at
2.15)
Theodore Gull, NASA, Goddard Space
Flight Center, Astrophysics Science Division, USA
Eta Carinae: A Box of Puzzles ... Some
Solved by 3D Modeling, Others Await
December 9th,
2010, 14:15
Marianne Vestergaard,
DARK, Niels Bohr Institute, Copenhagen,
Denmark
Accreting
Supermassive Black Holes Across Cosmic History
December 13th,
2010, 10:30 (Monday 10.30 -
Nobel Laureate Lecture - Lecture hall A, Physics)
Konstantin
Novoselov, The School of Physics & Astronomy,
University of Manchester, Uk
GRAPHENE: Carbon's New
Phase
December
16th, 2010, 14:15
Jan Conrad, Fysikum, Stockholm
University, Sweden
Indirect Detection of Dark
Matter - Status and Perspectives
Seminar coordinators:
David
Hobbs & Dainis Dravins
[deputy]
Lund Observatory, Box 43, SE-221 00 Lund, Sweden
Visiting address: Sölvegatan 27
Phone: +46 46 22 27300, Fax: +46 46 22 24614
Publisher: Bengt
Söderström
E-mail: webmaster@astro.lu.se
Last updated:
DH, 2010 August 5th
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