Post-main-sequence planetary system evolution [PDF]
The fates of planetary systems provide unassailable insights into their formation and represent rich cross-disciplinary dynamical laboratories. Mounting observations of post-main-sequence planetary systems necessitate a complementary level of theoretical
Dimitri Veras
doaj +4 more sources
The saccade main sequence revised: A fast and repeatable tool for oculomotor analysis. [PDF]
Saccades are rapid ballistic eye movements that humans make to direct the fovea to an object of interest. Their kinematics is well defined, showing regular relationships between amplitude, duration, and velocity: the saccadic ’main sequence’.
Gibaldi A, Sabatini SP.
europepmc +2 more sources
A planet within the debris disk around the pre-main-sequence star AU Microscopii. [PDF]
AU Microscopii (AU Mic) is the second closest pre-main-sequence star, at a distance of 9.79 parsecs and with an age of 22 million years 1 . AU Mic possesses a relatively rare 2 and spatially resolved 3 edge-on debris disk extending from about 35 to 210 ...
Plavchan P+86 more
europepmc +3 more sources
An inverse-linear logistic model of the main sequence [PDF]
A model of the main sequence is proposed based on the logistic function. The model’s fit to the peak velocity-amplitude relation resembles an S curve, simulta- neously allowing control of the curve’s asymptotes at very small and very large amplitudes, as
Andrew Duchowski+7 more
doaj +2 more sources
A Main Sequence for Quasars [PDF]
The last 25 years saw a major step forward in the analysis of optical and UV spectroscopic data of large quasar samples. Multivariate statistical approaches have led to the definition of systematic trends in observational properties that are the basis of
Paola Marziani+9 more
doaj +2 more sources
Speed-accuracy tradeoffs influence the main sequence of saccadic eye movements [PDF]
Several studies have proposed that an optimal speed-accuracy tradeoff underlies the stereotyped relationship between amplitude, duration and peak velocity of saccades (main sequence).
Leslie Guadron+2 more
doaj +2 more sources
New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit [PDF]
We present new models for low-mass stars down to the hydrogen-burning limit that consistently couple atmosphere and interior structures, thereby superseding the widely used BCAH98 models.
I. Baraffe+4 more
semanticscholar +3 more sources
SDSS-IV MaNGA: Spatially Resolved Star Formation Main Sequence and LI(N)ER Sequence [PDF]
We present our study on the spatially resolved Hα and M* relation for 536 star-forming and 424 quiescent galaxies taken from the MaNGA survey. We show that the star formation rate surface density ( ), derived based on the Hα emissions, is strongly ...
B. Hsieh+22 more
semanticscholar +6 more sources
A Noninteracting Galactic Black Hole Candidate in a Binary System with a Main-sequence Star [PDF]
We describe the discovery of a solar neighborhood (d = 468 pc) binary system with a main-sequence sunlike star and a massive noninteracting black hole candidate. The spectral energy distribution of the visible star is described by a single stellar model.
S. Chakrabarti+12 more
semanticscholar +1 more source
Surface Rotation and Photometric Activity for Kepler Targets. II. G and F Main-sequence Stars and Cool Subgiant Stars [PDF]
Dark magnetic spots crossing the stellar disk lead to quasiperiodic brightness variations, which allow us to constrain stellar surface rotation and photometric activity.
A. R. G. Santos+3 more
semanticscholar +1 more source