Search

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.

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.

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.

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

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.

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.

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.

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.

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.