Distance - courses.psu.edu
Dissipation and heating in solar wind turbulence: from the macro to
DISSERTATION
Dispersive Extinction Theory of Redshift
disparition de l*humanité: et alors ?
disks surviving the radiation pressure of radio pulsars
Disks - Osservatorio di Arcetri
Disk Structure
Disk Galaxies: Structural Components
Disk evolution: dust and gas\*
Disk and wind interaction in the young stellar object MWC 297
Disk
Disentangling planetary orbits from stellar activity in radial
Discussion Session A: “Evidence”
Discussion Activity #13
Discussion about Noise Equivalent Power and its use for photon
Discussion 17
Discrimination of exoplanetary and stellar radio flux
Discrete surveys: past, present and future
Discovery probability of transiting extragalactic planets and
