Search

22 May 2012: HR 4796A; Schneideret al. 2009), clumps (e.g.ε Eri; Greaves et al. ... ESA’s DARWIN mission concept)is extensively discussed in Defrère et al. (2010).

18 Sep 2007: Reference Targets Nstar Ndisks %850 mm, 1 j rms. (mJy). Wyatt et al. ... 2006b),IRAS 60 mm excess (Chen et al. 2006), andage (Smith et al.

5 Oct 2007: Magellan, Meyer et al. (2001) found excess emission suggesting the presence of circumstellar. ... performed (Watson et al. 2004). The reduction and analysis of the spectra was conducted with.

6 Apr 2010: Holland et al. 1998; Greaves et al. 2005; inscattered light imaging, e.g. ... range from highly reddened carbon stars or Class II YSO’sLisse et al.

1 Aug 2012: 2004). In order to avoid time-consuming peak-up, theobservatory was operated in IRS spectral mapping mode wherea 2 3 raster (spatial dispersion) centered on the star wasperformed (Watson et al. ... 5–2.0 μm) particles of the Tempel 1 ejecta (Lisse et

19 Feb 2010: It is an ex-tension of the model described in Wyatt et al. ... We take other model parametersfrom the best fit model of Wyatt et al.

29 Apr 2008: Send offprint requests to: R. Smith. have been resolved (e.g., Holland et al. ... 2005), thoughtto be there because this is a young (12Myr, Zuckerman et al.

23 Feb 2012: 1. The Astrophysical Journal, 747:93 (25pp), 2012 March 10 Lisse et al. ... was performed, with 1 cycle of 6 s integration at eachposition (Watson et al.