000002484 001__ 2484
000002484 005__ 20160701171706.0
000002484 037__ $$aASTROimport-641
000002484 100__ $$aBlomme, R.
000002484 245__ $$aStellar Winds of Early-Type Stars
000002484 260__ $$c2002
000002484 520__ $$aPrevious work on IRAS observations showed inhomogen- eities ("clumping") to be present in the wind of some early- type stars. To study this in more detail, we obtained ISOPHOT data at 60, 90 and 160 m for 1 LBV, 2 B-type stars and 5 Wolf-Rayets. The ISOPHOT data consist of P32 oversampled maps, which show a strong and highly structured background (infrared cirrus) on which the weak signal of the star is super- posed. The data still need to be reduced and corrected for the background before fluxes can be derived. 
000002484 700__ $$a Runacres, M. C.
000002484 773__ $$c67$$pPhotometric Mapping with ISOPHOT using the "P32" Astronomical Observation Template$$v482$$y2002
000002484 85642 $$ahttp://esoads.eso.org/abs/2002ESASP.482...67B
000002484 905__ $$apublished in
000002484 980__ $$aNONREF