Studying Stellar Systems with Classical Pulsators

Date Issued
2018
Author(s)
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Abstract
Classical Cepheids and RR Lyrae are very important primary distance indicators and stellar population tracers, thanks to the relations between pulsation properties and intrinsic stellar parameters. Through the theoretical prediction of these relations as well as through the direct comparison between predicted and observed light and radial velocity variations, we are able to constrain the stellar properties of the investigated pulsating stars and their host stellar populations, as well as to study the dependence on chemical composition.
Coverage
The RR Lyrae 2017 Conference. Revival of the Classical Pulsators: from Galactic Structure to Stellar Interior Diagnostics
All editors
Smolec, R.; Kinemuchi, K.; Anderson, R.I.
Series
Volume
6
Start page
55
Conferenece
The RR Lyrae 2017 Conference. Revival of the Classical Pulsators: from Galactic Structure to Stellar Interior Diagnostics
Conferenece place
Niepołomice, Poland
Conferenece date
17-21 September, 2017
Uri
Url
Issn Identifier
2545-1022
Ads BibCode
2018pas6.conf...55M
Rights
open.access
File(s)
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Thumbnail Image
Name

v6p55.pdf

Description
Pdf editoriale
Size

8.23 MB

Format

Adobe PDF

Checksum (MD5)

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