tPIC2.2 supplies a list of 217,741 stars for PLATO's LOPS2 field, including 202,315 FGK dwarfs/subgiants and 15,037 M dwarfs with uniformly estimated temperatures, radii, and masses.
Title resolution pending
5 Pith papers cite this work. Polarity classification is still indexing.
5
Pith papers citing it
citation-role summary
method 1
citation-polarity summary
verdicts
UNVERDICTED 5roles
method 1polarities
use method 1representative citing papers
SPHERE H-band observations resolve a smaller, thicker, brighter disk with inner spirals around V721 CrA and a larger disk with a dark lane around BN CrA, both consistent with their locations in the CrA star-forming region.
Sco-Cen shows abrupt jumps and plateaus in velocity dispersion correlated with star formation bursts, indicating isotropic expansion, inside-out propagation at 5-6 km/s, and stellar feedback as the primary driver.
Binary disruption and relaxation models explain the zone of avoidance and thermal eccentricities in S-star orbits around the Galactic center black hole.
RTGen applies post-processing Monte Carlo radiative transfer to six hydrodynamic galaxy simulations to compute dust temperatures, SEDs, continuum images, and molecular line emission while testing the effects of dust modeling choices.
citing papers explorer
-
The PLATO Input Catalogue of targets (tPIC) for the first Long Pointing Field
tPIC2.2 supplies a list of 217,741 stars for PLATO's LOPS2 field, including 202,315 FGK dwarfs/subgiants and 15,037 M dwarfs with uniformly estimated temperatures, radii, and masses.
-
Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): V721 CrA and BN CrA have wide and structured disks in polarised IR
SPHERE H-band observations resolve a smaller, thicker, brighter disk with inner spirals around V721 CrA and a larger disk with a dark lane around BN CrA, both consistent with their locations in the CrA star-forming region.
-
The evolution of velocity dispersion in the Sco-Cen OB association
Sco-Cen shows abrupt jumps and plateaus in velocity dispersion correlated with star formation bursts, indicating isotropic expansion, inside-out propagation at 5-6 km/s, and stellar feedback as the primary driver.
-
The S stars' zone of avoidance in the Galactic center
Binary disruption and relaxation models explain the zone of avoidance and thermal eccentricities in S-star orbits around the Galactic center black hole.
-
Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D
RTGen applies post-processing Monte Carlo radiative transfer to six hydrodynamic galaxy simulations to compute dust temperatures, SEDs, continuum images, and molecular line emission while testing the effects of dust modeling choices.