Search

28 Oct 2013: Brown etal. 2012, Simpson et al. 2011, Triaud et al. 2010, Winn etal. ... von Braun K. et al., 2011, ApJ 729, L26. Watson C.A.

23 Jul 2014: primordial protoplanetary disk (Watson et al. ... The system wassubsequently observed with theSpitzer Infra-Red Spectrograph(IRS, Houck et al.

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).

21 Jan 2014: 1990;. c 0000 RAS. 2 G. M. Kennedy et al. Muzerolle et al. ... 4.8. Schneider et al. (2013)report a detection in the XMM-Newton Serendipitous Source Cat-alog (Watson et al.

14 Nov 2013: 8 Matthews et al. Table 6Relative Flux Contributions from the Belt and Halo. ... 2009).The suggestion that the entire HR 8799 system may be. coplanar is consistent with the results of Watson et al.(2011) and Greaves et al.

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.

29 Apr 2016: 2009;Su et al. 2013; Kennedy & Wyatt 2014). For cool debrisdiscs, i.e. ... Interferometric measurements of Vega, the archetype of de-bris disk systems (Aumann 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.

2 Nov 2015: 2014) with Spitzer/IRACand CoRoT simultaneously over 30 days. Morales-Calderón et al. ... 2013) with the relative abundancesof solar elements as estimated by Caffau 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.

29 Oct 2013: 1995) and later a giant planet (Chauvin et al.2004) via this method. ... Le Bouquin et al. 2009; Watson et al.2011; Kennedy et al.

4 Dec 2014: They are less massive thanprotoplanetary discs ( 1 M of dust; Panić et al. ... 2008), Monnier et al. (2012, Vega), Mamajek (2012,Fomalhaut) and Zuckerman et al.

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

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).

2 Jul 2014: 2001; Mayor & Queloz 2012) or transit surveys e.g. CoRoT(Auvergne et al. ... 2010; Rodler et al. 2011; Giacobbe et al. 2012;Anglada-Escudé & Tuomi 2012).

25 Nov 2015: Continued. c 2002 RAS, MNRAS000, 1–18. 6 Z. H. Draper et al. ... of the disk is morewidely distributed than a simple ring (Booth et al.

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.

5 May 2017: As argued by de Wit et al. [40] a picture is emerging in which RZ Pscis surrounded by a massive young version of our own asteroid belt, in which planetesimalsare continually ... 675 1.5] 1.05, where anextinction of 0.3 per unit airmass was used, derived

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.

10 Feb 2021: 2018), and the additional 5 browndwarfclass II sources discussed in Sanchis et al. ... Further detailed discussion of the class II sourcesis included in Ansdell et al.

7 Jan 2014: 2006) sur-veys and Herschel DEBRIS2 (Matthews et al. 2013b) andDUNES3 (Eiroa et al. ... stars are statistically indistinguishable,a result supported by DUNES data (Eiroa 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.