Poster Open Access

Mapping M Dwarf Metallicities

DiTomasso, Victoria; Schmidt, Sarah J.


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  <identifier identifierType="DOI">10.5281/zenodo.2641980</identifier>
  <creators>
    <creator>
      <creatorName>DiTomasso, Victoria</creatorName>
      <givenName>Victoria</givenName>
      <familyName>DiTomasso</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0003-0741-7661</nameIdentifier>
      <affiliation>Leibniz Institute for Astrophysics Potsdam</affiliation>
    </creator>
    <creator>
      <creatorName>Schmidt, Sarah J.</creatorName>
      <givenName>Sarah J.</givenName>
      <familyName>Schmidt</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-7224-7702</nameIdentifier>
      <affiliation>Leibniz Institute for Astrophysics Potsdam</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Mapping M Dwarf Metallicities</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2019</publicationYear>
  <dates>
    <date dateType="Issued">2019-04-16</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Poster</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/2641980</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.2641979</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/eslab53</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/zenodo</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;We use distances derived from Gaia parallaxes cross-matched with SDSS, WISE and 2MASS photometry to assemble a sample of approximately 2 million M dwarfs, defined as stars with SDSS colors redder than r-i = 0.3 and i-z = 0.2. Previous work has found relations between SDSS r-z and WISE W1-W2 colors and the effective temperature and metallicities of cool stars (3550-4200 K). Using our sample and these previously derived relationships, we measure these stars&amp;#39; metallicities and effective temperatures. We calculate the metallicity distribution gradient as a function of galactic height for M dwarfs within 1000 pc of the Sun, which ultimately lends insight to the kinematic and chemical evolution of the Galaxy.&lt;/p&gt;</description>
    <description descriptionType="Other">{"references": ["Cheng, J. Y., et al. Metallicity Gradients in the Milky Way Disk as Observed by the SEGUE Survey", "Davenport, J. R. A. &amp; Dorn-Wallenstein, T. Z., Photometric Metallicities for Low-mass Stars with Gaia and WISE", "Garcia Perez, A. E., et al. (2015) ASPCAP: The APOGEE Stellar Parameter and Chemical Abundances Pipeline", "Green, G. M., et al. (2018) Galactic reddening in 3D from stellar photometry - an improved map", "Hartkopf, W.I. &amp; Yoss, K.M. (1982) A Kinematic and Abundance Survey at the Galactic Poles", "Schlesinger, K.J., et al. (2014) The Vertical Metallicity Gradient of the Milky Way Disk: Transitions in [\u03b1/Fe] Populations", "Schmidt, S. J., et al. (2016) Examining the relationships between colour, Teff, and [M/H] for APOGEE K and M dwarfs", "Woolf, V. M. &amp; West, A. A. (2012) The M dwarf problem in the Galaxy"]}</description>
  </descriptions>
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