Poster Program PD3/EX4

PD3/EX4

Formation and Dynamical Evolution of Planetary Systems (co-organized)
Session details
Oral Program
 / Thu, 12 Sep, 09:00–12:30  / 14:00–15:30  / Room Uranus - Chemistry C. Ingold Lecture Theatre
Poster Program
 / Attendance Thu, 12 Sep, 17:45–19:15  / Poster Area
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Attendance Time: Thursday, 12 Sep, 17:45–19:15
Poster Area
Chairperson: Caroline Terquem
P150
EPSC2013-950
Global models of planetary system formation
G. A. L. Coleman and R. P. Nelson

P151
EPSC2013-363
Gas Accretion by Giant Planets: a study with 3D inviscid hydrodynamical simulations
J. Szulágyi, A. Crida, and F. Masset

P152
EPSC2013-211
Dead zone inner edge dynamics in protoplanetary disks
J. Faure, S. Fromang, and H. Latter

P153 EPSC2013-407
Are Planetary Systems Filled to Capacity? (withdrawn)
J. Fang and J. L. Margot

P154
EPSC2013-746
A new high-precision [Fe/H] calibration for M dwarfs in the visible: a tool to explore the star-planet connection.
V. Neves, X. Bonfils, N.C. Santos, X. Delfosse, B.-O. Demory, G. Torres, T. Forveille, F. Allard, and S. Udry

P155
EPSC2013-230
Titanium and vanadium oxides as possible tracers of C/O in protoplanetary disks
M. Ali Dib, O. Mousis, G. S. Pekmezci, J. I. Lunine, N Madhusudhan, and J.-M. Petit

P156
EPSC2013-38 | Presentation
PFO-CFO Hypothesis of Solar System Formation: the presolar star as the only source of chemical elements for the Solar System
E. A. Kadyshevich and V.E. Ostrovskii

P157
EPSC2013-145 | Presentation
PFO-CFO Hypothesis of Solar System formation: the notion of the Sun-like stars and their transformations
V.E. Ostrovskii and E.A. Kadyshevich

P158
EPSC2013-59 | Presentation
Where does the huge orbital a.m. of solar and exoplanets come from? Evidence in both arenas that they get it during during nebula-borne construction, the property of new insight on the physics of gravitation
M.F. Osmaston

P159
EPSC2013-290 | Presentation
Angular momenta of collided rarefied preplanetesimals
S.I. Ipatov

P160
EPSC2013-291
Effects of Exoplanet Planetesimal Carbon Chemistry on Habitability
T. V. Johnson, O. Mousis, J. I. Lunine, and N. Madhusudhan

P161
EPSC2013-300
The effect of resonance order decrease in N+2 body problem
A. Rosaev

P162 EPSC2013-310
On circumpulsar disk characteristics (withdrawn)
C. Grimani

P163
EPSC2013-571
An explanation of forms of planetary orbits and estimation of angular shift of the Mercury' perihelion using the statistical theory of gravitating spheroidal bodies
A.M. Krot

P164
EPSC2013-919
Tensor equations in slightly aspherical configurations: get peace of mind with TenGSHui
A. Trinh

P165
EPSC2013-1098
Is the gap-opening criterion that was derived for laminar discs applicable to gravitationally unstable discs?
M. Malik, F. Meru, and M. R. Meyer