Seyfert Galaxies: A Perspective with the Infrared Space Observatory (ISO)
We present data from the Infrared Space Observatory (ISO) of a complete set of Seyfert galaxies (Seyfert 1 and Seyfert 2) in a wavelength range seldom explored...
Most previous work studying the possible relation between the presence of non-axisymmetric structures such as bars and rings in a galaxy, and the presence of...
Shape and Mutual Orbit Modeling of Binary Near-Earth Asteroid 2020 BX<SUB>12</SUB>
Approximately 15% of the near-Earth asteroid (NEA) population are estimated to be binary systems. 54 binaries have Arecibo radar observations; 2020 BX 12 is one...
Shape models and dynamical properties of basaltic asteroids outside the dynamical Vesta family
Through numerical modeling, Nesvorny et al. (2008) showed that asteroids can migrate due to Yarkovsky drift and resonances to outside of the boundaries of the...
Shape, size, physical properties and nature of low-perihelion near-Earth asteroid (3200) Phaethon
We apply the convex inversion method to the new optical data obtained by six instruments together with the already existing observations and derive convex shape...
Shaping massive galaxies: their morphology and kinematics at z = 1-3
Massive (M_* ≥ 10^{11} M_&sun;) galaxies at high redshift (z ≥ 1.5) remain mysterious objects. Their extremely small sizes (effective radii of 1-2 kpc) make...