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10 Nov 2017: Note left-right excursions corresponding to core contraction and onset of new burning phase.

6 Nov 2017: is adjusted, to take account of the fusion processes, to give composition at t=t0δt- new composition used to solve the stellar structure equations again- sequence repeats through lifetime of the

17 Nov 2017: Historically, until last fifteen years, “objective-prism” spectra employed. • New wide-field photometric surveys allow accurate (few percent, i.e.

10 Nov 2017: 2016 AJ 151 51 doi:10.3847/0004-6256/151/3/51. New, 2016, 27µm image shows extensions to the NW and SW as seen in shorter wavelength observations – Blackbody temperature

18 Oct 2017: Bahcall and E.E. Salpeter). New Interpretation of Extragalactic Radio Sources. Nat 229, 312 (1971) (errata, p. ... Pacini). New Evidence on Long-term Behaviour of Her X-1. Nat 244, 212 (1973) (with A.C.

16 Nov 2017: Structure & Evolution of Stars 27. New HST observations at ultraviolet wavelengths –sensitive to [Fe/H] variations.

18 May 2017: inclination and position angle), eccentricity, and argument of periastron. We now use these new results to discuss. ... Our new ALMA image is the first conclusive observational evidence for apocenter glow.

26 Sep 2017: parameters of their molecular gas component. Here we. report on new ALMA observations of seven disks, which. ... results as lower limits (Tab. 1). 5. DISCOVERY OF THREE NEW GASEOUSDEBRIS DISKS.

13 Nov 2017: Class 0/I sources: see below). Here, new theoreticalstudies are charting the chemical processing of cloud abundance patterns that are tobe expected during the early phases of disc assembly (Drozdovskaya et

11 Sep 2017: 2016). A new. episode of dips has started in May- June, 2017 (Boyajian. ... 2004), WISE (Wright et al. 2010), and new. optical observations, which were taken more than 10.

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.