The Comparison of the Classical Keplerian Orbit Elements, Non-Singular Orbital Elements (Equinoctial Elements), and the Cartesian State Variables in Lagrange Planetary Equations with J2 Perturbation: Part I [PDF]
Two semi-analytic solutions for a perturbed two-body problem known as Lagrange planetary equations (LPE) were compared to a numerical integration of the equation of motion with same perturbation force.
Jung Hyun Jo+3 more
doaj +2 more sources
Statistical distributions of orbital elements of interstellar meteors [PDF]
The suggestion on the interstellar origin of the definitely hyperbolic meteors is justified.
A. K. Markina, L. Ya. Skoblikova
doaj +2 more sources
Orbital elements of barium stars formed through a wind accretion scenario [PDF]
Taking the total angular momentum conservation in place of the tangential momentum conservation, and considering the square and higher power terms of orbital eccentricity e, the changes of orbital elements of binaries are calculated for wind accretion ...
J. H. Liu+3 more
openalex +4 more sources
Orbital Elements and Individual Component Masses from Joint Spectroscopic and Astrometric Data of Double-line Spectroscopic Binaries [PDF]
We present orbital elements, orbital parallaxes, and individual component masses for 14 spatially resolved double-line spectroscopic binaries derived doing a simultaneous fit of their visual orbit and radial velocity curve.
Jennifer Anguita-Aguero+3 more
semanticscholar +1 more source
Improved Elements of the Orbits of Asteroids
Kiyotsugu Hirayama, Kaoru AKIYAMA
openalex +6 more sources
On the Determination of the Orbital Elements of Eclipsing Variable Stars. I.
Henry Norris Russell
openalex +2 more sources
Elements of the Orbit of Comet Wells [PDF]
A. Graham
openalex +3 more sources
A set of orbital elements to fully represent the zonal harmonics around an oblate celestial body [PDF]
This work introduces a new set of orbital elements to fully represent the zonal harmonics problem around an oblate celestial body. This new set of orbital elements allows to obtain a linear system for the unperturbed problem and, in addition, a ...
D. Arnas, R. Linares
semanticscholar +1 more source
Local Orbital Elements for the Circular Restricted Three-Body Problem
The Keplerian orbital elements make up a set of parameters that uniquely describe a two-body trajectory. Once perturbations are imposed on two-body dynamics, one often studies the time evolution of the orbital elements.
Luke T. Peterson, D. Scheeres
semanticscholar +1 more source
Primary extranodal diffuse large B‐cell lymphoma: Molecular features, treatment, and prognosis
One‐third of DLBCL arises from extranodal organs and is challenging to manage. Molecular features are critical to elucidate the differences in clinical features, predict the disease prognosis, and improve effective targeted therapeutic strategies. Abstract Diffuse large B‐cell lymphoma (DLBCL) is the most common subtype of non‐Hodgkin's lymphoma and ...
Si‐Yuan Chen+3 more
wiley +1 more source