The polarization of the infrared source CRL 2688 /the EGG Nebula/

Details The polarization of the infrared source CRL 2688 /the EGG Nebula/ The polarization of the infrared source CRL 2688 /the EGG Nebula/

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...204l..25s&link_type=abstract

Astrophysical Journal, vol. 204, Feb. 15, 1976, pt. 2, p. L25-L28. Research supported by the University of Kansas.

Astronomy and Astrophysics

Astronomy

15

Astronomical Spectroscopy, Infrared Astronomy, Nebulae, Polarization (Waves), Graphite, Interstellar Extinction, Light Scattering, Polarized Electromagnetic Radiation, Silicates

Scientific paper

Polarization observations of CRL 2688 (the Egg Nebula) show the
polarization to vary from 40 percent at 3800 A to 52 percent near 9400
A. Observations of both components are also given. Polarization and
reddening models seem to indicate graphite rather than silicate
particles and a column density of the order of 1 billion per sq cm.

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