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An Analysis of the Shapes of Interstellar Extinction Curves. VI. The Near-IR Extinction Law

  • Authors: E. L. Fitzpatrick and D. Massa

FITZPATRICK & MASSA 2009 The Astrophysical Journal 699 1209.

  • Provider: AAS Journals

Caption: Figure 4.

Power-law exponent β vs. E( BV) (top panel) and R( V) (bottom panel) for the "β-variable" fits from Table 3. The dotted horizontal lines show the value β = 1.84. The filled triangle in the lower panel represents the sight line to the star ρ Oph from Martin & Whittet (1990). The 1σ error bars are based on fits to the Monte Carlo simulations of the data and the noise model.

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