ism extinction curveeldora.as.arizona.edu/~yshirley/arizona/ast300b/ast300b...some form of...

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2/10/20 1 ISM Extinction Curve Notice this is inverse wavelength à Or “wavenumber” Whittet – Dust in Galactic Environment 217.5 nm Effect of R V on Extinction Curve Notice this is inverse wavelength à Or wavenumber

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Page 1: ISM Extinction Curveeldora.as.arizona.edu/~yshirley/Arizona/AST300B/AST300B...some form of sp2-bonded carbon material. 23.3.2 Silicate Features at 9.7 pm and 18 pm There is a conspicuous

2/10/20

1

ISM Extinction Curve

Notice this is inverse wavelength àOr “wavenumber”

Whittet – Dust in Galactic Environment

217.5 nm

Effect of RV on Extinction Curve

Notice this is inverse wavelength àOr wavenumber

Page 2: ISM Extinction Curveeldora.as.arizona.edu/~yshirley/Arizona/AST300B/AST300B...some form of sp2-bonded carbon material. 23.3.2 Silicate Features at 9.7 pm and 18 pm There is a conspicuous

2/10/20

2

Typical Al Table

Adapted from Rieke & Lebofsky 1986

Column Density vs. E(B-V) Relation

Rachford et al. 2009

(5.94 +/- 0.37) X 1021 atoms cm-2 mag-1

Page 3: ISM Extinction Curveeldora.as.arizona.edu/~yshirley/Arizona/AST300B/AST300B...some form of sp2-bonded carbon material. 23.3.2 Silicate Features at 9.7 pm and 18 pm There is a conspicuous

2/10/20

3

Infrared Extinction Curve

Notice we’ve switched back to àjust wavelength

Falls off like a power-law tpfar-IR/radio

Extinction Mapping : Using background star color excesses to measure Al