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13 Nov 2018: Credit: V. Belokurov (Cambridge, UK and CCA, New York, US) based on the images by Marcus and Gail Davies and Robert Gendler. ... Torrealba (Academia Sinica, Taiwan), V. Belokurov (Cambridge, UK and CCA, New York, US) based on the image by ESO/S.

18 May 2018: The Hexenberg Cake - a new take on an old favourite.

24 Jan 2018: This work was supported by the European Community Research and Training Nework. The Physics of the Intergalactic Medium. Links. Send e-mail to.

5 Jul 2018: 1950s. AlpherGamowHermanHayashi. BBN CMB. = New Physics? BBN CMB. = New Physics?

29 Mar 2018: All other elements are created in (or by) stars, becoming available to form new stars, planets, and people. • ... Context • Activities • Download our app! Gaia science: learning how to learn Science results – new sources, supernovae directly to

6 Jul 2018: Credit: V. Belokurov (Cambridge, UK and CCA, New York, US) based on the image by ESO/Juan Carlos Muñoz. ... Credit: V. Belokurov (Cambridge, UK and CCA, New York, US) and Gaia/ESA.

30 Jul 2018: New data have been taken and the results are includedhere for Eri and 110 Her. ... The detection around 110 Her is also confirmed witha new measurement of 34357 zodis.

24 Jan 2018: New instruments, such as Dazle, are being developed to look for high-z Lyman-alpha emitters.

11 Oct 2018: 3.32). The force due to this new potential is:. FΛ = VΛr.

31 Jul 2018: in prep). New science yield estimates based on HOSTSupper limits are currently under study. ... New. Space-based infrared interferometry to study exoplanetary atmospheres 11. 10 100 1000Angular separation [mas].

25 Oct 2018: This is alsoreferred to as the ‘quantum gravity limit’ because it involves new physicallaws that unify quantum physics (which describes the strong and weaknuclear forces and the electromagnetic force) and gravity

9 Nov 2018: 2018). The study by Rappaport et al. involved examining allphotometric data from the Kepler mission by eye, lookingfor new dimming events which had not been detected by thePlanet Hunters citizen scientist ... Comparing these numbers to Figure 14 ofWyatt

6 Nov 2018: In both cases, we find no evidence for. new physics. The Planck results for base CDM are in good agreement with baryon acoustic oscillation data and with the JLA sample of

9 Mar 2018: report the discovery of two new disks,in the GJ 433 and GJ 649 systems. ... These observations were obtained with the aim of. discovering new debris disks in these systems, and in search of.

8 Oct 2018: Bruno was born in 1548,five years after Copernicus died. Between the years 1582 and 1592 he wasthe one who persistently, openly and actively spread the news about the“universe” that

6 Nov 2018: sources of noise in microwave satel-lite communications at Bell Laboratories in New Jersey.4 Their discoverywas announced alongside the interpretation of the CMB as relic thermalradiation from the Big Bang

22 Nov 2018: In Sec. 2, we start by introducing the new concept ofshielded discs that can explain massive CO gas discs as beingof secondary origin rather than hybrid. ... 3) and gas from new ALMA observations andwhether there is enough C0 observed to produce this

23 Oct 2018: Inthe early 1980s a new subclassification of supernovae emerged: SNe of typeI were further divided into type Ia and type Ib depending on the presence.

31 Jul 2018: In this paper we present new ALMA observations ofHD 107146 in both band 6 and 7 (1.1 and 0.86 mm). ... In 2 we present the new ALMA observations of thedust continuum and line emission of HD 107146.

30 Oct 2018: Key: p(n, γ)d p n d γ. BBN stops at 7Li because no stable nucleus of mass number 5 or 8 existsand thus no new nuclei can be formed

31 Jul 2018: Observatory, Carlsbad, California, USA7Bar J Observatory, New Smyrna Beach, Florida, 32168, USA8Angel Peaks Observatory, Cotopaxi, Colorado, 81223, USA9Karen Observatory, 12 Handley Drive, Padgate, Warrington, Cheshire, WA2 0GN, UK10Department of

22 Nov 2018: Extensions of the standard model ofparticle physics known as supersymmetry (SUSY) entertain the existenceof a large number of new particles, the lightest of which would be stable.None have yet been ... Itmust also be said that the supersymmetric WIMP

5 Apr 2018: 0.270.10, where. these new debiased parameters are consistent with the. biased ones. ... The main difference between Fig. 5 and Fig. 3 is. that a new lower envelope of detectability appears at.

30 Jul 2018: MNRAS 000, 1–23 (2015) Preprint 30 July 2018 Compiled using MNRAS LATEX style file v3.0. Using warm dust to constrain unseen planets. Amy Bonsor1, Mark C. Wyatt1, Quentin Kral1, Grant Kennedy2,3, Andrew. Shannon4,5 and Steve Ertel61Institute of

30 Jul 2018: 2656 Q. Kral et al. Figure 8. New probability map: similar to Fig. ... Figure 9. New ejection map: similar to Fig. 3, but for an inclined distribu-tion of comets (see Section 3.5 for more details).

2 Apr 2018: Our overall detection. rate is 18%, including four new detections, among which are the first three around Sun-like stars and the first two. ... preset to a new star. During the nodding cycles the. beams from both apertures are brought to

19 Feb 2018: 2013)reported a higher rate of 20.2 2 per cent. This result was de-rived from new IR data obtained with the PACS camera (Poglitschet al. ... Five of these sources are identified by Eiroaet al. (2013) as new discs discovered by Herschel.

15 May 2018: spreading material flows beyond the Roche limit, it coagulates into new (mi-nor) planets in a process analogous to the ongoing formation of moonlets at the outer edge ofSaturn’s rings. ... Roche limit is gradually quenched by PRdrag, eventually

14 Jun 2018: MNRAS 000, 1–21 (2017) Preprint 14 June 2018 Compiled using MNRAS LATEX style file v3.0. Modelling the KIC8462852 light curves: compatibility of the dipsand secular dimming with an exocomet interpretation. M. C. Wyatt1?, R. van Lieshout1, G. M.

31 Jul 2018: MNRAS 000, 1–23 (0000) Preprint 6 June 2018 Compiled using MNRAS LATEX style file v3.0. Scattering of exocomets by a planet chain: exozodi levelsand the delivery of cometary material to inner planets. Sebastian Marino1?, Amy Bonsor1, Mark C.