Poster Open Access

Magneto-chronology of nearby Sun-like stars

Gondoin, P.


Dublin Core Export

<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:creator>Gondoin, P.</dc:creator>
  <dc:date>2021-09-28</dc:date>
  <dc:description>Nearby Sun-like stars are prime targets of the PLATO mission for the detection and characterization of exo- planets and possibly exo-Earths. Understanding the formation history and determining the age of these sample stars (and their planetary systems) is thus essential.

The chromospheric emission in the cores of the Ca II H &amp; K lines of late-type dwarfs is a well-known indicator of magnetic activity that decreases with increasing stellar age. I used this indicator to investigate the formation history of nearby G- and early K-type stars with origins at galactocentric distances similar to that of the region where the Sun was born.</dc:description>
  <dc:identifier>https://zenodo.org/record/5534700</dc:identifier>
  <dc:identifier>10.5281/zenodo.5534700</dc:identifier>
  <dc:identifier>oai:zenodo.org:5534700</dc:identifier>
  <dc:relation>doi:10.5281/zenodo.5534699</dc:relation>
  <dc:relation>url:https://zenodo.org/communities/plato2021</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights>
  <dc:title>Magneto-chronology of nearby Sun-like stars</dc:title>
  <dc:type>info:eu-repo/semantics/conferencePoster</dc:type>
  <dc:type>poster</dc:type>
</oai_dc:dc>
77
64
views
downloads
All versions This version
Views 7777
Downloads 6464
Data volume 16.5 MB16.5 MB
Unique views 7070
Unique downloads 6161

Share

Cite as