Results 71 to 80 of about 3,349 (181)
The quest for Magrathea planets
Context. Planetary formation might occur at different stages of the stellar evolution. In particular, theoretical studies have been focusing on addressing whether formation can occur around compact binaries that evolved beyond the main sequence ...
Nigioni Arianna +4 more
doaj +1 more source
Kozai-Lidov cycles towards the limit of circumbinary planets
In this paper we answer a simple question: can a misaligned circumbinary planet induce Kozai-Lidov cycles on an inner stellar binary? We use known analytic equations to analyse the behaviour of the Kozai-Lidov effect as the outer mass is made small.
Martin, David V. +1 more
core +1 more source
Probing the presence of planets in transition discs' cavities via warps: the case of TW Hya [PDF]
We are entering the era in which observations of protoplanetary discs properties can indirectly probe the presence of massive planets or low mass stellar companions interacting with the disc.
Facchini, Stefano +2 more
core +3 more sources
New Pulse Timing Measurements of the sdBV Star CS 1246
CS 1246 is a hot subdwarf B star discovered in 2009 to exhibit a single, large-amplitude radial pulsation. An O-C diagram constructed from this mode revealed reflex motion due to the presence of a low-mass M dwarf, as well as a long-term trend consistent
Hutchens Zackary L. +7 more
doaj +1 more source
Circumbinary Planet Formation in the Kepler-16 system. I. N-body Simulations
The recently discovered circumbinary planets (Kepler-16 b, Kepler-34 b, Kepler-35 b) represent the first direct evidence of the viability of planet formation in circumbinary orbits.
Holman +12 more
core +1 more source
Migration of planets in circumbinary discs [PDF]
Aims. The discovery of planets in close orbits around binary stars raises questions about their formation. It is believed that these planets formed in the outer regions of the disc and then migrated through planet-disc interaction to their current location.
Thun, Daniel, Kley, Wilhelm
openaire +2 more sources
Young protostellar binary systems, with expected ages less than ∼10 ^5 yr, are little modified since birth, providing key clues to binary formation and evolution. We present a first look at the young, Class 0 binary protostellar system R CrA IRAS 32 from
Frankie J. Encalada +21 more
doaj +1 more source
A new approach for probing circumbinary disks
Circumbinary disks are considered to exist in a wide variety of astrophysical objects, e.g., young binary stars, protoplanetary systems, and massive binary black hole systems in active galactic nuclei (AGNs).
Atsuo T. Okazaki +19 more
core +1 more source
The Nature of Transition Circumstellar Disks II. Southern Molecular Clouds [PDF]
Transition disk objects are pre-main-sequence stars with little or no near-IR excess and significant far-IR excess, implying inner opacity holes in their disks. Here we present a multifrequency study of transition disk candidates located in Lupus I, III,
Allen, Lori E. +7 more
core +2 more sources
Empirical Stability Criteria for 3D Hierarchical Triple Systems. I. Circumbinary Planets
In this work we revisit the problem of the dynamical stability of hierarchical triple systems with applications to circumbinary planetary orbits. We derive critical semimajor axes based on simulating and analyzing the dynamical behavior of 3 × 10 ^8 ...
Nikolaos Georgakarakos +3 more
doaj +1 more source

