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SAE-PD-Seq: sequence autoencoder-based pre-training of decoder for sequence learning tasks

Signal, Image and Video Processing, 2021
Jyostna Devi Bodapati
exaly  

A precise asteroseismic age and metallicity for HD 139614: a pre-main-sequence star with a protoplanetary disc in Upper Centaurus–Lupus

Monthly Notices of the Royal Astronomical Society, 2021
Tim Bedding   +2 more
exaly  

The Evolution of Pre-Main-Sequence Stars

1999
The location of optically visible Pre-Main-Sequence (PMS) stars in the H-R diagram combined with the use of theoretical evolutionary tracks have played a central role in stellar evolution studies since the initial work of Hayashi, Cameron and Iben in the early ′60s.
openaire   +1 more source

The Pisa pre-main sequence database

2010
In recent years new observational data of pre-main sequence stars (pre-MS) with metallicity lower than solar have been made available; the study of the star formation regions requires comparison between theoretical models and observational data to assign masses and ages to the stars.
Tognelli E.   +2 more
openaire   +1 more source

Asteroseismology of pre-main sequence stars

2008
More than 30 years ago the first pulsating pre-main sequence (PMS) stars have been discov- ered. Since then, pulsations in 18 Herbig Ae stars and 18 members of young open clusters were detected and detailed asteroseismic investigations were conducted for some of them. We describe our latest results in this field.
Zwintz, Konstanze   +2 more
openaire   +2 more sources

PRE-MAIN-SEQUENCE EVOLUTION

2018
S. SOFIA   +3 more
openaire   +1 more source

New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit

Astronomy and Astrophysics, 2015
Isabelle Baraffe   +2 more
exaly  

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