Results 1 to 10 of about 3,775,618 (221)

A Main Sequence for Quasars [PDF]

open access: yesFrontiers in Astronomy and Space Sciences, 2018
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   +7 more sources

An inverse-linear logistic model of the main sequence [PDF]

open access: yesJournal of Eye Movement Research, 2017
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

Post-main-sequence planetary system evolution [PDF]

open access: yesRoyal Society Open Science, 2016
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   +2 more sources

Speed-accuracy tradeoffs influence the main sequence of saccadic eye movements [PDF]

open access: yesScientific Reports, 2022
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

Blue Stragglers After the Main Sequence [PDF]

open access: yesThe Astrophysical Journal, 2008
We study the post-main sequence evolution of products of collisions between main sequence stars (blue stragglers), with particular interest paid to the horizontal branch and asymptotic giant branch phases.
Alison Sills   +22 more
core   +5 more sources

Entropy Production of Main-Sequence Stars [PDF]

open access: yesEntropy, 2015
The entropy production (inside the volume bounded by a photosphere) of main-sequence stars is calculated based on B–V photometry data. The entropy-production distribution function and the dependences of entropy production on temperature and luminosity ...
Leonid M. Martyushev, Sergey N. Zubarev
doaj   +4 more sources

Pre-main-sequence Lithium Depletion [PDF]

open access: yes, 2004
In this review I briefly discuss the theory of pre-main-sequence (PMS) Li depletion in low-mass (0 ...
A. Ford   +35 more
core   +5 more sources

The Pre--Main-Sequence of A-type stars [PDF]

open access: yesProceedings of the International Astronomical Union, 2004
Young A-type stars in the pre--main-sequence (PMS) evolutionary phase are particularly interesting objects since they cover the mass range (1.5-4 solar ma sses) which is most sensitive to the internal conditions inherited during the protostellar phase ...
Marconi, Marcella, Palla, Francesco
core   +4 more sources

Abundances on the Main Sequence of Omega Centauri [PDF]

open access: yesThe Astrophysical Journal, 2007
Abundance ratios of carbon, nitrogen and strontium relative to iron, calculated using spectrum synthesis techniques, are given for a sample of main sequence and turnoff stars that belong to the globular cluster omega Centauri.
Alonso A.   +14 more
core   +5 more sources

The Ages of Pre-main-sequence Stars [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1998
The position of pre-main-sequence or protostars in the Hertzsprung--Russell diagram is often used to determine their mass and age by comparison with pre-main-sequence evolution tracks.
Alexander   +45 more
core   +4 more sources

Home - About - Disclaimer - Privacy