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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.

20 Feb 2024: lanet that was later disco v ered (Mouillet et al. 1997 ; Lagranget al. ... 2006 ), (14) Watson et al. ( 2011 ), (15) Sepulveda & Bowler ( 2022 ), (16) Mamajek & Bell ( 2014 ), (17) Plavchan et al. (

8 Jan 2019: P] 5. Jan. 201. 9. 2 S. Marino et al. Backman et al. ... Moreover, HD 131835 is known to have large amountsof gas (Moór 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.

23 Nov 2021: The method was refined byMiotello et al. (2016), accounting self-consistently forisotope selective dissociation. ... a few times the value of the minimummass Solar Nebula, Trapman et al., 2017).

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 2018: However, a trend of disc incidencewith stellar age has been observed (Su et al. ... 3054 B. Sibthorpe et al. 3.2.1 Distribution of observed disc properties.

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.