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18 Oct 2017: Jones). The 13 billion year bang. New Scientist, 72, 512 (1976) (20th Anniversary issue). ... Galactic nuclei and quasars, New Scientist, 80, 188 (1978). Are galaxies here to stay?

24 Oct 2017: mass element will continue to rise if less dense than new surroundings and convection will occur. ... drdT. H. H. µγ. γ. ρµ. γγ. γγ. =. =. <. When energy transport via convection must replace equation for the temperature gradient using new

18 Oct 2017: A new look at the Cosmos. The World in 1994, p144 (Economist publications). ... Daily Telegraph 13 Sept 1995. Reminiscences of S Chandrasekhar. New Scientist 30 Sept 1995.

9 Oct 2017: The Sun has spectral class G2. In recent years, new observations allow detection of the faintest stars and brown dwarfs, resulting in extension of the scheme to include types L and

2 Nov 2017: Follow-up Hubble Space Telescope observations in Adams et al. Existing HST precursor images (top), new 2015 images (middle) and near-infrared images (bottom).

16 Nov 2017: more tightly constrained via observations?• From the upper end, new studies of supernovae progenitors, as in Star of the Week #2, now making progress• From the lower end, use observations of

15 Oct 2017: The new line-width determination scheme is the key to the project.From Clewley et al., 2002, MNRAS, 337, 87.

22 Oct 2017: Energy released given by Einstein’s formula E=mc2, where “m”=Δm the difference in mass between the constituent light nuclei and the nucleus of the new element. •

13 Oct 2017: What are the new values of apparent and absolute mag-nitude? Q6c: The supernova remnant, in the shape of a ring, is expanding with aspeed v = 10, 000 km s1.

10 Nov 2017: Fusion in shell via p-p chain and CNO cycle becomes the new energy source for the star. •

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

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.

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

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

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.

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

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: 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