Search

23 Dec 2017: on Exoplanets, Université de Montréal, Montréal, QC H3C 3J7, Canada84Department of Astronomy, Columbia University, 550 West 120th Street, New York, NY 10027, USA85Department of Physics and Astronomy, 12 Physics Hall, Iowa ... These colors

21 Nov 2017: MNRAS 000, 1–16 (2017) Preprint 21 November 2017 Compiled using MNRAS LATEX style file v3.0. A dearth of small particles in the transiting materialaround the white dwarf WD 1145017. S. Xu1?, S. Rappaport2, R. van Lieshout3, A. Vanderburg4, B. Gary5

18 May 2017: 2012).However, only complete millimetre imaging of the ringcan constrain its azimuthal morphology and eccentricity.We achieved the latter through a new 1.3 mm mosaicobtained with ALMA and described in ... with a β Pictoris-likegaseous environment

5 May 2017: In orderto obtain the best disc constraints, in our analysis we combine newALMA band 7 observations and new data at 0.85 mm from the Sub-millimetre Common-User Bolometer Array

5 May 2017: 36–38]). As a young K0Vtype star with no evidence for gas accretion and a strong infrared (IR) excess, this system appearsunique among UXors and may provide new information on the ... observing season). If events repeat three times, then a new dimming

5 May 2017: We present a new semi-analyticalequivalent of the numerical model of Kral et al. ... We in-cluded the four new CO ALMA detections by Lieman-Sifryet al.