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électronique et électrotechnique - iate.europa.eu
An active k0 iv--v star and a hot white dwarf (euve j0702+129) in a wide binary... The International Ultraviolet Explorer spectra show continuum emission from a hot white dwarf (T eff = 30 \Gamma 40; 000 K) and a rising contribution from the K0 star at 2500 A....
électronique et électrotechnique - core.ac.uk - PDF: citeseerx.ist.psu.edu
Iso-lws observations of herbig ae/be stars... The adopted model computes the continuum emission from star, circumstellar gas and dust arranged in a spherical geometry....
Sensitive radio observations of high redshift dusty qsos... We detect radio continuum emission from four of the sources: BRI 0952\Gamma0115, BR 1202\Gamma0725, LBQS 1230+1627B, and BRI 1335\Gamma0417....
Astronomy and astrophysics on outflowing viscous disc models for be stars... It is found that the outflowing viscous disc models can reproduce the observed IR continuum emission....
Radio continuum emission as a star formation tracer: bridging the spatial scalesRadio continuum emission has been demonstrated to be an excellent tracer of recentstar formation, yet current understanding remains empirical, and is primarily basedupon integrated ...

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