Results 21 to 30 of about 327,633 (295)
The signatures of the parental cluster on field planetary systems
Due to the high stellar densities in young clusters, planetary systems formed in these environments are likely to have experienced perturbations from encounters with other stars.
Cai, Maxwell Xu +2 more
core +1 more source
Extra-solar planetary systems [PDF]
The discovery of extra-solar planets has captured the imagination and interest of the public and scientific communities alike, and for the same reasons: we are all want to know the answers to questions such as “Where do we come from?” and “Are we alone?” Throughout this century, popular culture has presumed the existence of other worlds and extra ...
J, Najita, W, Benz, A, Hatzes
openaire +2 more sources
The ALMA survey to Resolve exoKuiper belt Substructures (ARKS)
Context. CO gas has been detected in ~20 debris discs, typically classified as CO-poor or CO-rich. We present observations of the CO-rich HD 121617 debris disc as part of the ALMA survey to Resolve exoKuiper belt Substructures (ARKS). Aims.
Brennan A. +26 more
doaj +3 more sources
Towards planetary health systems: a manifesto for a revised quadruple aim for healthcare improvement
Non-technical summary Healthcare systems significantly impact the environment, which in turn affects human health. To address this, we propose to revise a popular framework for healthcare improvement, by introducing the advancement of planetary health ...
Alessio Perilli +4 more
doaj +1 more source
“Free-floating, non-deuterium-burning, substellar objects” are isolated bodies of a few Jupiter masses found in very young open clusters and associations, nearby young moving groups, and in the immediate vicinity of the Sun.
José A. Caballero
doaj +1 more source
DIVISION III: PLANETARY SYSTEMS SCIENCE [PDF]
The meeting was opened by Ted Bowell, president, at 11 am. The 2006 Division III meetings were reviewed by Guy Consolmagno, secretary; as the minutes of those meetings have already been published, they were assumed to be approved.
Edward L. G. Bowell +17 more
openaire +4 more sources
Microlensing Searches for Exoplanets
Gravitational microlensing finds planets through their gravitational influence on the light coming from a more distant background star. The presence of the planet is then inferred from the tell-tale brightness variations of the background star during the
Yiannis Tsapras
doaj +1 more source
Observations and modeling of the transiting exoplanets XO-2b, HAT-P-18b, and WASP-80b [PDF]
We present photometric observations and transit solutions of the exoplanets XO-2b, HAT-P-18b and WASP 80b. Our solution of the XO-2b transit gave system parameters whose values are close to those of the previous studies. The solutions of the new
Kjurkchieva Diana P. +2 more
doaj +1 more source
To assess the permeability structure of the oceanic lithosphere, we analyzed the field-based vein distribution and geometry in the Wadi Haymiliyah area of the Oman ophiolite.
Genya Sakamoto +4 more
doaj +1 more source
Exoplanet Predictions Based on Harmonic Orbit Resonances
The current exoplanet database includes 5454 confirmed and candidate planets observed with the Kepler mission. We find 932 planet pairs from which we extract distance and orbital period ratios.
Markus J. Aschwanden, Felix Scholkmann
doaj +1 more source

