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.

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.

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.

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.

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.

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.

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.

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.

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.

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).

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.

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