Anagram & Information om | Engelska ordet WN

Exempel på hur man kan använda WN i en mening

• The ratio between the two types of Wolf–Rayet stars (WC stars and WN stars) in IC 10 is very different from the ratio in other galaxies in the Local Group, which may be somehow due to the starburst nature of the galaxy.
• The (WN) - Resistance Nest at the Château-de-Tailleville (de la colonie) was a unique ‘platoon-sized’ position, incorporating standard concrete (Verstärkt Feltmessig: Vf Type 2) gun casemates, with well-sited observation and crewed fighting positions.
• In the course of these investigations, a payoff from former Cognos sales executive Joseph Lally in the amount of $600,000 USD was found to have been made to Vitale's company WN Advisors.
• 14; WN 6: Variations in E major on the air "Der Schweizerbub: Steh'auf, steh'auf o du Schweitzer Bub", a.
• Its fossils, holotype WN V-6, were found in a bonebed in lacustrine limestone exposed on the seafloor off the coast of the town of Bale on the Istrian peninsula in Croatia by Dario Boscarolli during the 1980s, and described in 1998 by Dalla Vecchia.
• For the first time, the Caprice no longer had a unique dashboard; instead, the WN gained the same all-new interior, dashboard, sports steering wheel and corporate MyLink infotainment system from the VF generation Holden Calais.
• Developed Monoclonal antibodies against JE, Dengue, WN, Chikungunya, Influenza and respiratory syncytial viruses (RSV).
• England: HB Tristram (Oxford University), CG Wade (Oxford University), CE Chapman (Cambridge University), WN Bolton (Blackheath), A Rotherham (Oxford University), HT Twynam (Richmond), JT Hunt (Manchester), CS Wooldridge (Blackheath), CJB Marriott (Cambridge University), Herbert Fuller (Cambridge University), EL Strong (Oxford University), WM Tatham (Oxford University), RSF Henderson (Blackheath), Charles Gurdon (Richmond), ET Gurdon (Richmond) capt.
• England: CH Sample (Cambridge University), WN Bolton (Blackheath), Andrew Stoddart (Blackheath), JJ Hawcridge (Bradford), A Rotherham (Oxford University), JH Payne (Broughton), Frank Moss (Broughton), G Harrison (Hull), AT Kemble (Liverpool), Charles Gurdon (Richmond), HJ Ryalls (New Brighton), CH Horley (Swinton), CS Wooldridge (Blackheath), GT Thomson (Halifax), ET Gurdon (Richmond) capt.
• England: AS Taylor (Blackheath), CG Wade (Oxford University), Arthur Evanson (Oxford University), WN Bolton (Blackheath), A Rotherham (Oxford University), JH Payne (Broughton), RS Kindersley (Oxford University), CS Wooldridge (Oxford University), Harry Vassall (Oxford University), Herbert Fuller (Cambridge University), Graham Standing (Blackheath), WM Tatham (Oxford University), Robert Henderson (Blackheath), GT Thomson (Halifax), ET Gurdon (Richmond) capt.
• England: AE Wood (Gloucester), WN Lapage (United Services), JGG Birkett (Harlequins), Henry Vassall (Oxford University), A Hudson (Gloucester), GV Portus (Blackheath), RH Williamson (Oxford University), R Gilbert (Devonport Albion), F Boylen (Hartlepool Rovers), TS Kelly (Exeter), CEL Hammond (Harlequins) capt.
• As an annex, it can be mentioned that the combinations ZD, ZE, ZF, WL, WN and some ZZ were only assigned to plates of this category in their early days.
• Empire Bairn was a member of Convoy WN 225 which sailed from Oban on 30 December 1941 and arrived at Methil, Fife on 2 January 1942.
• Stars with sufficiently strong mixing from the core to the surface, due to the very large convective core, high metallicity, or additional rotational mixing, may skip the LBV phase and evolve directly from the hydrogen-rich WNh phase to the hydrogen-poor WN phase.
• CycKies MS, Holsinger FC, Lee JJ, William WN, Glisson BS, Lin HY, Lewin JS, Ginsberg LE, Gillaspy KA, Massarelli E, Byers L, Lippman SM, Hong WK, El-Naggar AK, Garden AS, Papadimitrakopoulou V.
• Bakker MK, Kancherla V, Canfield MA, Bermejo-Sanchez E, Cragan JD, Dastgiri S, De Walle HEK, Feldkamp ML, Groisman B, Gatt M, Hurtado-Villa P, Kallen K, Landau D, Lelong N, Lopez Camelo JS, Martínez L, Morgan M, Mutchinick OM, Nembhard WN, Pierini A, Rissmann A, Sipek A, Szabova E, Tagliabue G, Wertelecki W, Zarante I, Mastroiacovo P.
• Ostroff RM, Bigbee WL, Franklin W, Gold L, Mehan M, Miller YE, Pass HI, Rom WN, Siegfried JM, Stewart A, Walker JJ, Weissfeld JL, Williams S, Zichi D, and Brody EN.
• According to evolution models, stars with initial masses of 25 to 40 M☉ have lifecycles of O → RSG → WN, and the evolution of WR 138a is consistent with the models.

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