output
19952026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions
Showing 1998 · astro-phShow all

7 papers · 2 filters

astro-ph1998★ 156 cited

The Accretion of Brown Dwarfs and Planets by Giant Stars -- I. AGB Stars

Lionel Siess, Mario Livio

We study the response of the structure of an asymptotic giant branch (AGB) star to the accretion of a brown dwarf or planet in its interior. In particular, we examine the case in w…

astro-ph1998★ 130 cited

Precession of collimated outflows from young stellar objects

C. Terquem, J. Eisloffel, J. Papaloizou +1

We consider several protostellar systems where either a precessing jet or at least two misaligned jets have been observed. We assume that the precession of jets is caused by tidal…

astro-ph1998★ 289 cited

The Palomar Testbed Interferometer

M. M. Colavita, J. K. Wallace

The Palomar Testbed Interferometer (PTI) is a long-baseline infrared interferometer located at Palomar Observatory, California. It was built as a testbed for interferometric techni…

astro-ph1998★ 42 cited

The response of accretion disks to bending waves: angular momentum transport and resonances

Caroline E. J. M. L. J. Terquem

We investigate the linear tidal perturbation of a viscous Keplerian disk by a companion star orbiting in a plane inclined to the disk. We consider m=1 perturbations with odd symmet…

astro-ph1998★ 74 cited

FU Orionis resolved by infrared long baseline interferometry at a 2-AU scale

F. Malbet, J. -P. Berger, M. M. Colavita +3

We present the first infrared interferometric observations of a young stellar object with a spatial projected resolution better than 2 AU. The observations were obtained with the P…

astro-ph1998

The Swallowing of Planets by Giant Stars

Lionel Siess, Mario Livio

We present simulations of the accretion of a massive planet or brown dwarf by an AGB star. In our scenario, close planets will be engulfed by the star, spiral-in and be dissipated…

astro-ph1998★ 209 cited

On the tidal interaction of a solar-type star with an orbiting companion: Excitation of g mode oscillation and orbital evolution

C. Terquem, J. C. B. Papaloizou, R. P. Nelson +1

We calculate the dynamical tides raised on a non-rotating solar-type star by a close stellar or planetary companion. Dissipation arising from a turbulent viscosity operating in the…