Poster Open Access

Decoding the Evolution of Young Stars: A Look at Magnetic Fields

Roberts, Max; Feiden, Gregory A.


MARC21 XML Export

<?xml version='1.0' encoding='UTF-8'?>
<record xmlns="http://www.loc.gov/MARC21/slim">
  <leader>00000nam##2200000uu#4500</leader>
  <datafield tag="653" ind1=" " ind2=" ">
    <subfield code="a">astronomy</subfield>
  </datafield>
  <datafield tag="653" ind1=" " ind2=" ">
    <subfield code="a">astrophysics</subfield>
  </datafield>
  <controlfield tag="005">20200120170306.0</controlfield>
  <controlfield tag="001">1052892</controlfield>
  <datafield tag="711" ind1=" " ind2=" ">
    <subfield code="d">28 October 2017</subfield>
    <subfield code="g">GRAM</subfield>
    <subfield code="a">2017 Georgia Regional Astronomy Meeting</subfield>
    <subfield code="c">Athens, GA, USA</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="u">University of North Georgia</subfield>
    <subfield code="0">(orcid)0000-0002-2012-7215</subfield>
    <subfield code="a">Feiden, Gregory A.</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2=" ">
    <subfield code="s">3855246</subfield>
    <subfield code="z">md5:e74e010b51ee98abc334390eba5c6253</subfield>
    <subfield code="u">https://zenodo.org/record/1052892/files/2017GRAM_Roberts.pdf</subfield>
  </datafield>
  <datafield tag="542" ind1=" " ind2=" ">
    <subfield code="l">open</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2017-11-17</subfield>
  </datafield>
  <datafield tag="909" ind1="C" ind2="O">
    <subfield code="p">openaire</subfield>
    <subfield code="o">oai:zenodo.org:1052892</subfield>
  </datafield>
  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="u">University of North Georgia</subfield>
    <subfield code="a">Roberts, Max</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Decoding the Evolution of Young Stars: A Look at Magnetic Fields</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
    <subfield code="u">https://creativecommons.org/licenses/by/4.0/legalcode</subfield>
    <subfield code="a">Creative Commons Attribution 4.0 International</subfield>
  </datafield>
  <datafield tag="650" ind1="1" ind2="7">
    <subfield code="a">cc-by</subfield>
    <subfield code="2">opendefinition.org</subfield>
  </datafield>
  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">&lt;p&gt;Poster presented at the 2017 Georgia Regional Astronomy Meeting at the University of Georgia (Athens, GA, USA).&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Abstract&lt;/strong&gt;&lt;br&gt;
Magnetic fields are hypothesized to affect the fundamental properties of young stars by increasing their size and cooling their surface temperature, as compared to stars without magnetic fields, at a given age. However, observational evidence supporting this hypothesis is scarce and is largely based on comparison of stellar evolution models that include effects from magnetic fields with a few select young stellar systems. Therefore, to expand on current knowledge, we present initial results from an effort to produce a large grid of magnetic stellar evolution models suitable for modeling young stellar systems of any age or metallicity. Once completed, the model grid will permit more rigorous tests of the hypothesis that magnetic fields affect the physical properties of young stars.&lt;/p&gt;</subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="n">doi</subfield>
    <subfield code="i">isVersionOf</subfield>
    <subfield code="a">10.5281/zenodo.1052891</subfield>
  </datafield>
  <datafield tag="024" ind1=" " ind2=" ">
    <subfield code="a">10.5281/zenodo.1052892</subfield>
    <subfield code="2">doi</subfield>
  </datafield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">poster</subfield>
  </datafield>
</record>
60
20
views
downloads
All versions This version
Views 6060
Downloads 2020
Data volume 77.1 MB77.1 MB
Unique views 5555
Unique downloads 1919

Share

Cite as