Description

We present stellar evolution models for 0.5 - 1.2 M[subscript ⊙] at scaled metallicities of 0.1 - 1.5 Z[subscript ⊙] and O/Fe values of 0.44 - 2.28 O/Fe[subscript ⊙]. The

We present stellar evolution models for 0.5 - 1.2 M[subscript ⊙] at scaled metallicities of 0.1 - 1.5 Z[subscript ⊙] and O/Fe values of 0.44 - 2.28 O/Fe[subscript ⊙]. The time dependent evolution of habitable zone boundaries are calculated for each stellar evolution track based on stellar mass, effective temperature, and luminosity parameterizations. The rate of change of stellar surface quantities and the surrounding habitable zone position are strong functions of all three quantities explored.

application/pdf

Download count: 0

Details

Contributors
Date Created
  • 2015-05-10
Resource Type
  • Text
  • Collections this item is in
    Identifier
    • Digital object identifier: 10.1088/0004-637X/804/2/145
    • Identifier Type
      International standard serial number
      Identifier Value
      0004-637X
    • Identifier Type
      International standard serial number
      Identifier Value
      1538-4357
    Note

    Citation and reuse

    Cite this item

    This is a suggested citation. Consult the appropriate style guide for specific citation guidelines.

    Truitt, Amanda, Young, Patrick A., Spacek, Alexander, Probst, Luke, & Dietrich, Jeremy (2015). A CATALOG OF STELLAR EVOLUTION PROFILES AND THE EFFECTS OF VARIABLE COMPOSITION ON HABITABLE SYSTEMS. ASTROPHYSICAL JOURNAL, 804(2), 0-0. http://dx.doi.org/10.1088/0004-637X/804/2/145

    Machine-readable links