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Interstellar Dust: Ultraviolet Extinction - a b...

Avatar for Karl Gordon Karl Gordon
August 05, 2019

Interstellar Dust: Ultraviolet Extinction - a biased review

A biased review of UV dust extinction curves for GeoffFest

Avatar for Karl Gordon

Karl Gordon

August 05, 2019
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  1. Interstellar Dust: Ultraviolet Extinction (a biased review) Karl D. Gordon

    GeoffFest Boulder, CO 5 Aug 2019 ISM@ST member [email protected] @karllark2000 karllark@github “Have Dust – Will Study” Slides on SpeakerDeck
  2. Plan • Intro • Milky Way UV extinction • Local

    Group UV extinction – LMC, SMC, M31, & M33 • Misc • Final Throughts
  3. Extinction (not Attenuation) • Extinction – Absorption and scattering out

    of the line-of-sight – Specific to a point source behind a screen of dust • (dust not too near the point source) – Extinction proportional to dust grain properties • Attenuation includes information not present in extinction – scattering into the line-of-sight – Star/dust geometry – Applies to galaxies, regions of galaxies, stars with circumstellar dust
  4. More CCM89 deviants Many are not CCM89 deviant Clayton &

    Hanson 1993, AJ, 105, 1880 Hanson & Clayton 1993, AJ, 106, 1947
  5. Final Thoughts • Geoff has a bunch of UV extinction

    papers • UV extinction story still being written • “True” R(V) dependent relationship – Sample selection critical • Local Group → just getting started – Need larger samples • Expanding beyond the UV – Optical: Derck’s talk – MIR: Spitzer (ongoing), NIR IRTF/SpeX (planned)
  6. Final Thoughts • Geoff has a bunch of UV extinction

    papers • UV extinction story still being written • “True” R(V) dependent relationship – Sample selection critical • Local Group → just getting started – Need larger samples • Expanding beyond the UV – Optical: Derck’s talk – MIR: Spitzer (ongoing), NIR IRTF/SpeX (planned)