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See detailK voprosou bidelenii fatsii zoubtchatogo moustié na materialakh pamyatnikov sredneï azii
Krivoshapkin, A.; Kolobova, K.; Pavlenok, K. et al

Scientific conference (2011)

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See detailK+ Production in a Cascade Model for High Energy Nucleus-Nucleus Collisions
Cugnon, Joseph ULiege; Lombard

in Nuclear Physics A (1984), 422

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See detailLe K-ABC utilisé avec des enfants trisomiques 21 : Un essai d’adaptation
Frenkel, Stéphanie ULiege; Bourdin, Béatrice; Vandromme, Luc

Conference (2001)

Detailed reference viewed: 26 (1 ULiège)
See detailLe K-ABC utilisé avec des enfants trisomiques 21 : Un essai d’adaptation
Frenkel, Stéphanie ULiege; Bourdin, Béatrice; Vandromme, luc

in Vivicorsi, Bruno; Collet, R. (Eds.) Handicap, cognition et prise en charge individuelle : des aspects de la recherche au respect de la personne (2005)

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See detailK-excess, an unexploited method for discovering red quasars
Nakos, T.; Willis, J.; Andreon, S. et al

Conference (2006, May 19)

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See detailK-shell photoabsorption and photoionization of trace elements. I. Isoelectronic sequences with electron number 3 <= N <= 11
Palmeri, P.; Quinet, Pascal ULiege; Bautista, M.A. et al

in Astronomy and Astrophysics (2016), 589

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See detailK-shell photoionization and photoabsorption of Ne, Mg, Si, S, Ar and Ca
Witthoeft, M; Bautista, M A; Mendoza, C et al

in Astrophysical Journal Supplement Series (2009), 182

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See detailK-shell photoionization of Na-like to Cl)like ions of Mg, Si, S, Ar and Ca
Witthoeft, M; Garcia, J; Kallman, T R et al

in Astrophysical Journal Supplement Series (2011), 192

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See detailK-shell photoionization of Nickel ions using R-matrix
Witthoeft, M C; Bautista, M A; Garcia, J et al

in Astrophysical Journal Supplement Series (2011), 196

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See detailK-type geomagnetic index nowcast with data quality control
Stankov, Stanimir; Stegen, Koen; Warnant, René ULiege

in Annals of Geophysics = Annali di Geofisica (2011), 54(3), 285-295

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See detailThe K1 beta-lactamase of Klebsiella pneumoniae.
Joris, Bernard ULiege; De Meester, F; Galleni, Moreno ULiege et al

in Biochemical Journal (1987), 243(2), 561-7

beta-Lactamase K1 was purified from Klebsiella pneumoniae SC10436. It is very similar to the enzyme produced by Klebsiella aerogenes 1082E and described by Emanuel, Gagnon & Waley [Biochem. J. (1986) 234 ... [more ▼]

beta-Lactamase K1 was purified from Klebsiella pneumoniae SC10436. It is very similar to the enzyme produced by Klebsiella aerogenes 1082E and described by Emanuel, Gagnon & Waley [Biochem. J. (1986) 234, 343-347]. An active-site peptide was isolated after labelling of the enzyme with tritiated beta-iodopenicillanate. A cysteine residue was found just before the active-site serine residue. This result could explain the properties of the enzyme after modification by thiol-blocking reagents. The sequence of the active-site peptide clearly established the enzyme as a class A beta-lactamase. [less ▲]

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See detailThe K2-ESPRINT Project I: Discovery of the Disintegrating Rocky Planet K2-22b with a Cometary Head and Leading Tail
Sanchis-Ojeda, R.; Rappaport, S.; Pallé, E. et al

in Astrophysical Journal (2015), 812(2), 112

We present the discovery of a transiting exoplanet candidate in the K2 Field-1 with an orbital period of 9.1457 hr: K2-22b. The highly variable transit depths, ranging from ∼0% to 1.3%, are suggestive of ... [more ▼]

We present the discovery of a transiting exoplanet candidate in the K2 Field-1 with an orbital period of 9.1457 hr: K2-22b. The highly variable transit depths, ranging from ∼0% to 1.3%, are suggestive of a planet that is disintegrating via the emission of dusty effluents. We characterize the host star as an M-dwarf with Teff ≃ 3800 K. We have obtained ground-based transit measurements with several 1-m class telescopes and with the GTC. These observations (1) improve the transit ephemeris; (2) confirm the variable nature of the transit depths; (3) indicate variations in the transit shapes; and (4) demonstrate clearly that at least on one occasion the transit depths were significantly wavelength dependent. The latter three effects tend to indicate extinction of starlight by dust rather than by any combination of solid bodies. The K2 observations yield a folded light curve with lower time resolution but with substantially better statistical precision compared with the ground-based observations. We detect a significant “bump” just after the transit egress, and a less significant bump just prior to transit ingress. We interpret these bumps in the context of a planet that is not only likely streaming a dust tail behind it, but also has a more prominent leading dust trail that precedes it. This effect is modeled in terms of dust grains that can escape to beyond the planet's Hill sphere and effectively undergo “Roche lobe overflow,” even though the planet's surface is likely underfilling its Roche lobe by a factor of 2. [less ▲]

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See detailKaberdoes
Vromans, Joseph ULiege

in Nederlands Van Nu (1993), 41(5),

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See detail"Kadenzen des ganzen Körpers" - Das Sich-Bewegen des Musikers.
Viehöver, Vera ULiege; Wunsch, Stephan

in Görling, Reinhold; Skrandies, Timo; Trinkaus, Stephan (Eds.) Geste - Bewegungen zwischen Film und Tanz (2009)

Detailed reference viewed: 102 (4 ULiège)
See detailKaffee, Cognac, Marmelade: Verfahrenstechnik im Alltagsleben
Pfennig, Andreas ULiege

Conference (2004, October 11)

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See detailKafka’s Circus Rings and Hunger Walls
Delville, Michel ULiege

in Armand, Louis (Ed.) Abolishing Prague (2015)

Detailed reference viewed: 42 (3 ULiège)