A Dust Shell around the Early Type Wolf-Rayet Star WR:19

Details A Dust Shell around the Early Type Wolf-Rayet Star WR:19 A Dust Shell around the Early Type Wolf-Rayet Star WR:19

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.247p..18w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 247, NO.2/NOV15, P. 18P, 1990

Astronomy and Astrophysics

Astronomy

13

Scientific paper

Infrared photometry of the WC4-type Wolf-Rayet star WR 19 (LS 3) in 1988-90 shows evidence for an expanding dust shell in its wind, similar to those observed from late-type WR stars like WR 48a (WC8), WR 140 (WC7 + 04) and WR 137 (WC 7+). This demonstrates that dust formation by Wolf-Rayet stars is not restricted to later WC subtypes and is more common than hitherto supposed.

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