Dust properties of [WCL] CSPNS

Details Dust properties of [WCL] CSPNS Dust properties of [WCL] CSPNS

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.275..103c&link_type=abstract

Astrophysics and Space Science, v. 275, Issue 1/2, p. 103-111 (2001).

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

The rather rare class of central stars of planetary nebulae that show Wolf-Rayet spectra have been a subject of great interest, particularly in the infrared, since their discovery in the late 1960s. I will focus on further peculiarities found within the past 1-2 years with the advent of infrared spectroscopy from ISO. Notably, these stars simultaneously betray the presence of regions of carbon-rich and oxygen-rich dust chemistry. I compare and contrast complete ISO spectra from 2 to 200 microns of a small sample of [WC9] to [WC11] central stars.

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