Published March 1990 | Version v1
Journal article

Optical identification of dust within the Crab Nebula's filaments

  • 1. Johns Hopkins Univ., Baltimore, MD (USA)
  • 2. Dartmouth College, Hanover, NH (USA)
  • 3. Colorado Univ., Boulder (USA)

Description

Optical continuum images of the Crab Nebula are presented which reveal numerous, small dark spots across the face of the Crab's amorphous synchrotron nebula. These spots range in size from being unresolved at 0.8-arcsec resolution to about 5 arcsec, exhibit Delta(m)4470 = 0.08-0.44, and are most visible in the shorter-wavelength continuum images. Comparisons with images taken using interference filters centered on various emission lines indicate that these dark features are coincident with forbidden O I, C I, and S II bright cores of selected filaments. This positional coincidence plus a wavelength dependence similar to that exhibited by conventional interstellar dust establishes the presence of dust within at least some of the Crab Nebula's filaments. 26 refs

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
351
Series
Astrophys. J.
Journal Page Range
L45-L48
ISSN
0004-637X
CODEN
ASJOA