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Variable stars in the VVV globular clusters. I. 2MASS-GC 02 and Terzan 10
(Institute of Physics Publishing, 2015-03)
The VISTA Variables in the Vía Láctea (VVV) ESO Public Survey is opening a new window to study inner Galactic globular clusters (GCs) using their variable stars. These GCs have been neglected in the past due to the ...
Constant of motion, Lagrangian and Hamiltonian of the gravitational attraction of two bodies with variable mass
(2007)
The Lagrangian, the Hamiltonian and the constant of motion of the gravitational attraction of two bodies when one of them has variable mass is considered. The relative and center of mass coordinates are not separated, and ...
Constant of motion, Lagrangian and Hamiltonian of the gravitational attraction of two bodies with variable mass
(2007)
The Lagrangian, the Hamiltonian and the constant of motion of the gravitational attraction of two bodies when one of them has variable mass is considered. The relative and center of mass coordinates are not separated, and ...
Pulsating low-mass white dwarfs in the frame of new evolutionary sequences. I: adiabatic properties
(Edp Sciences, 2014-09)
Context. Many low-mass white dwarfs with masses M∗/M⊙ ≲ 0.45, including the so-called extremely low-mass white dwarfs (M∗/M⊙ ≲ 0.20 − 0.25), have recently been discovered in the field of our Galaxy through dedicated ...
STUDY OF MASS-TRANSFER EFFICIENCY IN PERVAPORATION PROCESSES
(Elsevier Science BvAmsterdamHolanda, 1994)
Assessment of the structure and variability ofWeddell Sea water masses in distinct ocean reanalysis products
(2014)
We assessed and evaluated the performance of five ocean reanalysis products in reproducing essential hydrographic properties and their associated temporal variability for the Weddell Sea, Antarctica. The products used in ...