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...
Shock induced polarized hydrogen emission lines in omicron Ceti
We have performed a spectropolarimetric survey of the variable Mira star omicron Ceti along three pulsation cycles. We present those new data collected with the...
Shock-Induced Polarized Hydrogen Emission Lines in omicron Ceti
We have performed a spectropolarimetric survey of the variable Mira star omicron Ceti along three pulsation cycles. We present those new data collected with the...