Search

6 Jul 2016: IC Wales - Welsh news from the Western Mail.

16 Sep 2016: origin. Show that the new orbit of a dust grain with a given β has a semimajor axis ad andeccentricity ed given by.

6 Jul 2016: IC Wales - Welsh news as seen by The Western Mail etc. ... New Scientist - Weekly science news.

2 Dec 2016: We aim at discoveringand studying new such systems, to further expand our knowledge of how low-mass companions form and evolve.Methods. ... letter_HD206893. solving and characterising new debris discs never detected inscattered light (PI: Milli,

10 Nov 2016: Interestingly, weidentify a new feature of the disk: over the short axis of emission, one side of the disk is noticeably brighter. ... 2005) for details. Here, the new parameters are ǫλ (= 1.5a/λ when λ > 1.5a,but 1 otherwise; Greenberg 1979) the

13 Jul 2016: However, new probes of the inner disk may be the so-called “dipper” stars, whose optical and infrared light curvesexhibit episodic drops in flux consistent with extinction bytransiting dusty structures orbiting

23 Dec 2016: The outer disk is revealed in reprocessed archival Hubble Space Telescope NICMOSF110W images, as well as new coronagraphic H band images from the Very Large Telescope SPHEREinstrument. ... 2013, 2014; Mala-mut et al. 2014; Miles et al. 2016). Analyzing

21 Jul 2016: Research Council of Canada, 5071 West Saanich Rd, Victoria, BC, V9E 2E7, Canada4School of Physics, University of New South Wales, NSW, 2052, Sydney, Australia5ALMA Santiago Central Offices, Alonso de Crdova 3107, ... 2 OBSERVATIONS. The new data were

7 Jun 2016: This new model can be tested from its predictions for high resolutionALMA observations of C I. ... Two of them are new observations pre-sented here for the first time. •

29 Apr 2016: A summary of the observations, including the new obser-vations obtained for this programme in two observing runsduring 2015 (14/10-20/10 and 29/10-3/11), is given in

17 May 2016: New York, NY 10034, USA6Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1562, USA7Joint ALMA Observatory, Alonso de CÃşrdova 3107, 763-0355 Vitacura, Santiago, Chile8Exoplanets and Stellar ... al. 2013). After one

27 Jan 2016: This result sets a new record for high-contrast mid-infrared interferometricimaging and opens a new window on the study of planetary systems. ... New alignment. 8 Defrère et al. procedures will be developed during the science valida-tion phase to

23 Sep 2016: As one of the main goals of this work is to directly com-pare this new Band 6 CO J=2-1 dataset with the archivalCO J=3-2 Band 7 ... Finally, inSect. 3.3.3 we carry out a PV diagram comparison betweenthe new CO J=2-1 and the archival J=3-2 dataset.

7 Nov 2016: 1 Described in https://almascience.eso.org/news/notification-. always consistently centered on the star and neither were theoffsets always equal.

15 Mar 2016: Space Science Reviews manuscript No.(will be inserted by the editor). Insights into planet formation from debris disks. II. Giant impacts in extrasolar planetary systems. Mark C. Wyatt Alan P. Jackson. Received: date / Accepted: date. Abstract Giant

7 Oct 2016: arX. iv:1. 610. 0071. 4v1. [as. tro-. ph.E. P] 3. Oct. 201. 6. MNRAS 000, 1–25 (2016) Preprint 5 October 2016 Compiled using MNRAS LATEX style file v3.0. How to design a planetary system for different scattering. outcomes: giant impact sweet spot,