SIMBAD references

1994A&A...292..593P - Astronomy and Astrophysics, volume 292, 593-598 (1994/12-2)

Extended mid-infrared emission around Herbig Ae/Be stars.


Abstract (from CDS):

We have observed 7 young intermediate mass stars in the mid-infrared with two diaphragms of different sizes in order to detect extended emission. The mid-infrared part of the spectral energy distribution of HD97048, HD97300, and HD176386 is dominated by extended emission. The extended mid-infrared emission can best be explained with emission from large molecules and small grains in a dust shell with a large inner cavity devoid of small particles. The 4 strong mid-infrared sources of our sample (T CrA, R CrA, HD104237 and IRAS12496-7650) are dominated by emission within the smallest diaphragm (5.4") used in this work. When extended emission around Herbig Ae/Be stars is present, it contributes significantly to the mid-infrared luminosity and must be taken into account both in future observational and theoretical studies.

Abstract Copyright:

Journal keyword(s): stars: pre-main sequence - infrared: stars - stars: individual: HD97048 - stars: individual: HD97300 - stars: individual: HD176386

Simbad objects: 7

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