THE STAR FORMATION NEWSLETTER An electronic publication dedicated to early stellar evolution and molecular clouds No. 199 — 25 July 2009 Editor: Bo Reipurth (
[email protected]) Abstracts of recently accepted papers On the interplay between flaring and shadowing in disks around Herbig Ae/Be stars. B. Acke1, M. Min2, M. E. van den Ancker3, J. Bouwman4, B. Ochsendorf2, A. Juhasz4 and R. Waters1,2 1 Instituut voor Sterrenkunde, K.U.Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium 2 Sterrenkundig Instituut Anton Pannekoek, Universiteit van Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, the Netherlands 3 European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching bei Munchen, Germany 4 Max-Planck-Institut fur Astronomie, Konigstuhl 17, D-69117 Heidelberg, Germany E-mail contact: bram at ster.kuleuven.be Based on the SED, Herbig stars have been categorized into two observational groups, reflecting their overall disk structure: group I members have disks with a higher degree of flaring than their group II counterparts. We investigate the 5-35 um Spitzer IRS spectra of a sample of 13 group I sources and 20 group II sources. We focus on the continuum emission to study the underlying disk geometry. We have determined the [30/13.5] and [13.5/7] continuum flux ratios. The 7-um flux excess with respect to the stellar photosphere is measured, as a marker for the strength of the near-IR emission produced by the inner disk. We have compared our data to self-consistent passive-disk model spectra, for which the same quantities were derived. We confirm the literature result that the difference in continuum emission between group I and II sources can largely be explained by a different amount of small dust grains.