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Initial mass function

  • Quantifying the Uncertainties of Chemical Evolution Studies

    Quantifying the Uncertainties of Chemical Evolution Studies

  • –1– 1. the Salpeter Initial Mass Function the Initial Mass Function Is

    –1– 1. the Salpeter Initial Mass Function the Initial Mass Function Is

  • Measuring the Stellar Initial Mass Function

    Measuring the Stellar Initial Mass Function

  • Progenitor Mass Distribution for Core-Collapse Supernova Remnants in M31 and M33

    Progenitor Mass Distribution for Core-Collapse Supernova Remnants in M31 and M33

  • The Stellar Initial Mass Function and Beyond

    The Stellar Initial Mass Function and Beyond

  • Galactic Stellar and Substellar Initial Mass Function1

    Galactic Stellar and Substellar Initial Mass Function1

  • Protostar Mass Functions in Young Clusters

    Protostar Mass Functions in Young Clusters

  • A Study of Herbig Ae Be Star HD 163296: Variability in CO and OH Diana Lyn Hubis Yoder Clemson University, Dianahubis@Gmail.Com

    A Study of Herbig Ae Be Star HD 163296: Variability in CO and OH Diana Lyn Hubis Yoder Clemson University, [email protected]

  • Ast 777: Star and Planet Formation Pre-Main Sequence Stars and the IMF

    Ast 777: Star and Planet Formation Pre-Main Sequence Stars and the IMF

  • American Scientist the Magazine of Sigma Xi, the Scientific Research Society

    American Scientist the Magazine of Sigma Xi, the Scientific Research Society

  • Stellar Populations - Lecture IV

    Stellar Populations - Lecture IV

  • A Universal Stellar Initial Mass Function? a Critical Look at Variations

    A Universal Stellar Initial Mass Function? a Critical Look at Variations

  • On the Function Describing the Stellar Initial Mass Function

    On the Function Describing the Stellar Initial Mass Function

  • Etion in Herbig Ae/Be Stars

    Etion in Herbig Ae/Be Stars

  • Lecture 12: the Initial Mass Function (And a Little More About Debris Disks) Summary • Young Pre-Main Sequence Stars Are Surrounded by Disks of Gas and Dust

    Lecture 12: the Initial Mass Function (And a Little More About Debris Disks) Summary • Young Pre-Main Sequence Stars Are Surrounded by Disks of Gas and Dust

  • Stellar Masses

    Stellar Masses

  • The Relationship Between the Prestellar Core Mass Function and the Stellar Initial Mass Function

    The Relationship Between the Prestellar Core Mass Function and the Stellar Initial Mass Function

  • The History of Mass Dispersal Around Herbig Ae/Be Stars

    The History of Mass Dispersal Around Herbig Ae/Be Stars

Top View
  • The Initial Mass Function and Disk Frequency of the Ρ Ophiuchi Cloud: an Extinction-Limited Sample
  • The Universality of the Stellar Initial Mass Function
  • Herbig Ae/Be Stars
  • On the Mass Accretion Rates of Herbig Ae/Be Stars
  • Early Stages of Evolution and the Main Sequence Phase
  • Star Formation in the Ultraviolet
  • The Stellar Initial Mass Function 1
  • Gaia and Sigma Orionis from 20 Msol to 3 Mjup: the Most Complete And
  • The Impact of Binaries on the Stellar Initial Mass Function Pavel Kroupa and Tereza Jerabkova
  • The Origin of the Stellar Initial Mass Function
  • The Low Mass Stellar Population of the Orion OB1 Association And
  • Proto-Stellar Evolution Collapse
  • The Initial Mass Function
  • Star Formation Narrative Outline
  • Cloudlet Capture by Transitional Disk and FU Orionis Stars C
  • PDF, an Initial Mass Function for Individual Stars in Galactic Disks. I
  • Theory of Star Formation 1
  • Initial Mass Function


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