The potential of space observations for pulsating pre-main sequence stars
The first asteroseismic studies of pre-main sequence (pre-MS) pulsators have been conducted based on data from the space telescopes MOST and CoRoT with typical time bases of less than 40 days. With these data, a relation between the pulsational properties of pre-MS δ Scuti stars and their relative e...
Main Author: | Zwintz Konstanze |
---|---|
Format: | Article |
Language: | English |
Published: |
EDP Sciences
2017-01-01
|
Series: | EPJ Web of Conferences |
Online Access: | https://doi.org/10.1051/epjconf/201716003002 |
Similar Items
-
Tracing early stellar evolution with asteroseismology: pre-main sequence stars in NGC 2264
by: Zwintz Konstanze, et al.
Published: (2015-01-01) -
Observational studies of pre-main sequence stars
by: Hutchinson, Mark Gerard
Published: (1988) -
Opacity Effects on Pulsations of Main-Sequence A-Type Stars
by: Joyce A. Guzik, et al.
Published: (2018-06-01) -
FREQUENCY ANALYSIS OF PHOTOGRAPHIC OBSERVATIONS OF PULSATING STARS
by: V. P. Bezdenezhnyi
Published: (2017-04-01) -
Optical and infrared observations of pulsating variable stars
by: Fernley, J. A.
Published: (1985)