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1

Amatuzzi, Antonella. "Glaude Luython ou comment «apprendre parfaictement lire et parler francois» à travers les fables." Studi Francesi, no. 144 (XLVIII | III) (December 15, 2004): 555–66. http://dx.doi.org/10.4000/studifrancesi.37082.

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2

Honisch, Erika Supria. "Drowning Winter, Burning Bones, Singing Songs." Journal of Musicology 34, no. 4 (2017): 559–609. http://dx.doi.org/10.1525/jm.2017.34.4.559.

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In 1587 the Flemish composer Carolus Luython, employed by Holy Roman Emperor Rudolf II, published an unusual motet collection in Prague. Titled Popularis anni jubilus, the collection describes the sounds and rituals beloved by Central European peasants, recasting them as the ecstatic songs of rustic laborers (jubilus) famously celebrated by Saint Augustine in his Psalm commentaries. Highlighting the composer’s collaboration with the Czech cleric who wrote the motet texts, this study serves as a corrective to the interpretative frameworks that have broadly shaped discourses on Central European
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3

Humphreys, Roberta. "Willem J. Luyten." Physics Today 48, no. 4 (1995): 107. http://dx.doi.org/10.1063/1.2807997.

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4

Upgren, Arthur R. "Willem Jacob Luyten (1899-1994)." Publications of the Astronomical Society of the Pacific 107 (July 1995): 603. http://dx.doi.org/10.1086/133599.

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5

Bilwachs, Jan. "Die Konkordanzen der Carl Luythons Motetten Bellum insigne und Festa dies hodie." Musicologica Brunensia, no. 1 (2016): 37–45. http://dx.doi.org/10.5817/mb2016-1-3.

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6

Liebert, James, Conard C. Dahn, and David G. Monet. "The Luminosity Function of White Dwarfs in the Local Disk and Halo." International Astronomical Union Colloquium 114 (1989): 15–23. http://dx.doi.org/10.1017/s0252921100099267.

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The luminosity function (LF) and total space density of white dwarfs in the solar neighborhood contain important information about the star formation history of the stellar population, and provide an independent method of measuring its age. The first empirical estimates of the LF for degenerate stars were those of Weidemann (1967), Kovetz and Shaviv (1976) and Sion and Liebert (1977). The follow-up investigations made possible by the huge Luyten Palomar proper motion surveys, however, added many more faint white dwarfs to the known sample. While the number of known cool white dwarfs grew to ne
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7

Tyokyaa, K. R., and Tersoo Atsue. "POSITIONS AND STABILITY OF LIBRATION POINTS IN THE CIRCULAR RESTRICTED THREE-BODY PROBLEM WHEN THE BIGGER PRIMARY IS RADIATING AND OBLATING." FUDMA JOURNAL OF SCIENCES 4, no. 2 (2020): 523–31. http://dx.doi.org/10.33003/fjs-2020-0402-185.

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This paper investigates the positions and stability of libration points in the framework of the circular restricted three-body problem for the systems: Luyten726-8 and HD98800. The position of the third body lie in the plane almost directly above and below the center of the oblate primary. It is found that radiations and oblateness of the primary have destabilizing effects; the presence of any one or more of the latter makes weak the stabilizing ability of the former, consequently the overall effect is that the range of stability of the libration points decreases. Considering the range of stab
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8

Vanthemsche, G. "D. Luyten, Sociaal-economisch overleg in België sedert 1918." BMGN - Low Countries Historical Review 112, no. 1 (1997): 170. http://dx.doi.org/10.18352/bmgn-lchr.4448.

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9

Spence, Donald P. "Closing the Gap: Commentary On Luyten, Blatt, and Corveleyn." Journal of the American Psychoanalytic Association 54, no. 2 (2006): 619–25. http://dx.doi.org/10.1177/00030651060540022301.

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10

Oswalt, T. D., and E. M. Sion. "On the Separations of Common Proper Motion Binaries Containing White Dwarfs." International Astronomical Union Colloquium 114 (1989): 454–57. http://dx.doi.org/10.1017/s0252921100100065.

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Luyten [1,2] and Giclas et al. [3,4] list over 500 known common proper motion binaries (CPMBs) which, on the basis of proper motion and estimated colors, are expected to contain at least one white dwarf (WD) component, usually paired with a late type main sequence (MS) star. Preliminary assessments of the CPMBs suggest that nearly all are physical pairs [5,6]. In this paper we address the issue of whether significant orbital expansion has occurred as a consequence of the post-MS mass loss expected to accompany the formation of the WDs in CPMBs.Though the CPMB sample remains largely unobserved,
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11

Poveda, A., M. A. Herrera, C. Allen, G. Cordero, and C. Lavalley. "A Catalogue of Nearby Wide Binary and Multiple Stars." International Astronomical Union Colloquium 135 (1992): 299. http://dx.doi.org/10.1017/s025292110000659x.

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AbstractNo modern catalogue of wide binary and multiple systems (WBMS) exists for the region of the solar vicinity (stars nearer than ~22 pc), that include updated information on their membership to moving clusters and an age classification. With the aim of filling this gap, and also because of its importance for investigating the dynamical evolution of double and multiple systems, we have compiled a WBMS list extracted from the catalogues of nearby stars of Gliese (1969, also Gliese & Jahreiss 1979), as well as Luyten’s NLTT (Luyten 1979–1980, Luyten & Hughes 1980, see also Warren et
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12

Gould, Andrew, and Samir Salim. "Improved Astrometry and Photometry for the Luyten Catalog. I. Bright Stars." Astrophysical Journal 582, no. 2 (2003): 1001–10. http://dx.doi.org/10.1086/344818.

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13

Salim, Samir, and Andrew Gould. "Classifying Luyten Stars Using an Optical-Infrared Reduced Proper-Motion Diagram." Astrophysical Journal 575, no. 2 (2002): L83—L86. http://dx.doi.org/10.1086/342782.

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14

Chakraborty, Anindita, Ashutosh Narayan, and Amit Shrivastav. "Existence and stability of collinear points in elliptic restricted three body problem with radiating and oblate primaries." International Journal of Advanced Astronomy 4, no. 2 (2016): 95. http://dx.doi.org/10.14419/ijaa.v4i2.6523.

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The location of the collinear points in elliptical restricted three body problem, taking into account the effect of oblateness and radiation pressure of both primaries, has been obtained in this paper. Vinti's method has been exploited and the x-coordinates are obtained in the form of series solution. The linear stability has been investigated and it is found that the points are unstable in the Lyapunov's sense. The problem is also numerically explored taking into account two binary systems: Luyten-726 and Kruger-60.
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15

Klüter, J., U. Bastian, M. Demleitner, and J. Wambsganss. "Ongoing astrometric microlensing events of two nearby stars." Astronomy & Astrophysics 615 (July 2018): L11. http://dx.doi.org/10.1051/0004-6361/201833461.

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Context. Astrometric microlensing is an excellent tool to determine the mass of stellar objects. By measuring the astrometric shift of a background source star in combination with precise predictions of its unlensed position and of the lens position, gravitational lensing allows to one determine the mass of the lensing star with a precision of 1%, independently of any prior knowledge. Aims. Making use of the recently published Gaia Data Release 2 (Gaia DR2) we predict astrometric microlensing events by fore-ground stars of high proper motion passing by a background star in the coming years. Me
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16

Almond, Richard. "How Do We Bridge the Gap? Commentary On Luyten, Blatt, and Corveleyn." Journal of the American Psychoanalytic Association 54, no. 2 (2006): 611–18. http://dx.doi.org/10.1177/00030651060540020101.

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17

Vennes, Stéphane, and Adela Kawka. "Spectroscopic Identification of White Dwarfs in the New Luyten Two-Tenths Survey." Astrophysical Journal 586, no. 1 (2003): L95—L98. http://dx.doi.org/10.1086/374772.

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18

Lépine, S., M. M. Shara, R. M. Rich, A. Wittenberg, M. Halmo, and B. Bongiorno. "A new all-sky catalog of stars with large proper motions." Proceedings of the International Astronomical Union 3, S248 (2007): 74–77. http://dx.doi.org/10.1017/s1743921308018656.

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AbstractA new all-sky catalog of stars with proper motions μ > 0.15″ yr−1 is presented. The catalog is largely a product of the SUPERBLINK survey, a data-mining initiative in which the entire Digitized Sky Surveys are searched for moving stellar sources. Findings from earlier proper motions surveys are also incorporated. The new all-sky catalog supersedes the great historic proper motion catalogs assembled by W. J. Luyten (LHS, NLTT), and provides a virtually complete > 98% census of high proper motion stars down to magnitude R = 19.
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19

Dawson, P. C., and M. M. De Robertis. "High Proper Motion Stars. IV. Radial Velocities of 166 Luyten Half‐Second Stars." Publications of the Astronomical Society of the Pacific 117, no. 827 (2005): 1–12. http://dx.doi.org/10.1086/427790.

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20

Dos Santos, Mikeias Cardoso, and Maria do Socorro Carvalho. "O CORDEL: O JORNAL DO SERTÃO NORDESTINO." REVISTA DE LETRAS - JUÇARA 2, no. 2 (2018): 127–39. http://dx.doi.org/10.18817/rlj.v2i2.1767.

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O presente trabalho resulta da influência do Projeto de Extensão “A Literatura de Cordel na escola: ler, ouvir e escrever”, que objetiva promover as práticas de ouvir, ler e escrever por jovens do 1º Ano do Ensino Médio da escola Centro de Ensino Cônego Aderson Guimarães Júnior, Caxias-MA. O conhecimento poético e histórico dos cordelistas e a aproximação com questões de interesse público, que são relevantes como os problemas da sociedade: a decadência, a corrupção dos políticos, a falta de políticas públicas, os romances de moças donzelas em busca dos herois; as religiões; temas medievais; te
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21

Irwin, Jonathan M., David Charbonneau, Gilbert A. Esquerdo, et al. "Four New Eclipsing Mid M-dwarf Systems from the New Luyten Two Tenths Catalog." Astronomical Journal 156, no. 4 (2018): 140. http://dx.doi.org/10.3847/1538-3881/aad9a3.

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22

Bakos, Gaspar A., Kailash C. Sahu, and Peter Nemeth. "Revised Coordinates and Proper Motions of the Stars in the Luyten Half‐Second Catalog." Astrophysical Journal Supplement Series 141, no. 1 (2002): 187–93. http://dx.doi.org/10.1086/340115.

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23

Bues, I. "Results of a Spectrophotometric Survey of White Dwarf Suspects in the Solar Neighbourhood." International Astronomical Union Colloquium 114 (1989): 160–62. http://dx.doi.org/10.1017/s0252921100099504.

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320 blue stars of the Giclas and Luyten catalogues with positions δ 15° and magnitudes have been observed photometrically in UBVRI and Stromgren colours with the ESO lm telescope at La Silla in order to increase the number of close-by white dwarfs. From their Strömgren colours more than 120 stars belong to the white dwarf region. But, as outlined by Rupprecht and Bues (1983), a combination of the photometric systems and the combined two-colour diagrams (R−I)/(U−V) and (R−I) / (u−b) provide additional information on binary components. Fig.1 shows a sample in the (R−I)/(u−b)diagram. For (u−b) &l
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24

Duriez, Bart, Claudia Appel, and Dirk Hutsebaut. "The German Post-Critical Belief Scale: Internal and External Validity." Zeitschrift für Sozialpsychologie 34, no. 4 (2003): 219–26. http://dx.doi.org/10.1024/0044-3514.34.4.219.

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Abstract: Recently, Duriez, Fontaine and Hutsebaut (2000) and Fontaine, Duriez, Luyten and Hutsebaut (2003) constructed the Post-Critical Belief Scale in order to measure the two religiosity dimensions along which Wulff (1991 , 1997 ) summarized the various possible approaches to religion: Exclusion vs. Inclusion of Transcendence and Literal vs. Symbolic. In the present article, the German version of this scale is presented. Results obtained in a heterogeneous German sample (N = 216) suggest that the internal structure of the German version fits the internal structure of the original Dutch ver
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25

Narayan, A., A. Chakraborty, and A. Dewangan. "Nonlinear Stability of Oblate Infinitesimal in Elliptic Restricted Three-Body Problem Influenced by the Oblate and Radiating Primaries." Advances in Astronomy 2019 (February 27, 2019): 1–14. http://dx.doi.org/10.1155/2019/9480764.

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This work deals with the nonlinear stability of the elliptical restricted three-body problem with oblate and radiating primaries and the oblate infinitesimal. The stability has been analyzed for the resonance cases around ω1=2ω2 and ω1=3ω2 and also the nonresonance cases. It was observed that the motion of the infinitesimal in this system shows instable behavior when considered in the third order resonance. However, for the fourth order resonance the stability is shown for some mass parameters. The motion in the case of nonresonance was found to be unstable. The problem has been numerically ap
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26

Schott, Friedrich. "Comment on “The density jump across Little Bahama Bank” by J. Luyten and H. Stommel." Journal of Geophysical Research 90, no. C2 (1985): 3257. http://dx.doi.org/10.1029/jc090ic02p03257.

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27

Salim, Samir, and Andrew Gould. "Improved Astrometry and Photometry for the Luyten Catalog. II. Faint Stars and the Revised Catalog." Astrophysical Journal 582, no. 2 (2003): 1011–31. http://dx.doi.org/10.1086/344822.

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28

Braspenning, Gilbert. "Ahmed Essadki, Profetische gedichten, Strijdkreet van de aarde, riffijnse gedichten Alsmeer, uitgeverij Dabar-Luyten, 1997." Afrika Focus 18, no. 1-2 (2005): 119–24. http://dx.doi.org/10.1163/2031356x-0180102008.

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29

Wijngaert, M. van den. "D. Luyten, Burgers boven elke verdenking? Vervolging van economische collaboratie in België na de tweede wereldoorlog." BMGN - Low Countries Historical Review 113, no. 2 (1998): 281. http://dx.doi.org/10.18352/bmgn-lchr.4723.

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30

Singh, Nutan, Ashutosh Narayan, and B. Ishwar. "Trajectories of the infinitesimal mass around the triangular equilibrium points in elliptical restricted three bodies problem under oblate and radiating primaries for the binary systems." International Journal of Advanced Astronomy 3, no. 2 (2015): 107. http://dx.doi.org/10.14419/ijaa.v3i2.5304.

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<p>This paper describes the trajectory of the infinitesimal mass around L<sub>4</sub> of the triangular equilibrium points for the binary systems in the elliptical restricted three body’s problem (ERTBP), where both oblate primaries are radiating. The solutions for the perturbed motion in the vicinity of L<sub>4</sub> is given by u(f) and v(f) function .The stability of the infinitesimal mass around the triangular points is also studied by plotting u(f) and v(f) curve. It is found that radiation pressure, oblateness and eccentricity show a significant effect on th
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31

Pennington, R. L., R. M. Humphreys, and F. D. Ghigo. "The Minnesota Automated Plate Scanner: A New User Facility." Symposium - International Astronomical Union 133 (1988): 437–40. http://dx.doi.org/10.1017/s007418090013997x.

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The redevelopment of the Minnesota Automated Plate Scanner (APS) is complete and the system is being used as an astronomical visitor facility. The system consists of the original CDC-Luyten scanner with a new microprocessor-based motion control system, state of the art detection electronics, a PDP-11/60 data acquisition system with all relevant scanning parameters under software control, a Sun 3/110 computer for data reductions and a high speed link to the University of Minnesota Supercomputer Institute Cray 2 for reductions of very large projects. The redeveloped APS is among the fastest plat
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32

Singh, Nutan, and A. Narayan. "Analysis on nonlinear stability of the triangular libration points for radiating and oblate primaries in ER3BP." International Journal of Advanced Astronomy 5, no. 1 (2017): 50. http://dx.doi.org/10.14419/ijaa.v5i1.7104.

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In this paper we study the non linear stability of the triangular librations points in ER3BP considering both the primaries as radiating and oblate. The study is carried out near the resonance frequency satisfying the conditions in resonance as well as non resonance case. The study is conducted for various values of radiation pressure and oblateness parameters. It is observed that the case corresponds to the boundary region of the stability for the system Further, it is examined that the system experiences resonance at for different values of radiation pressures and oblateness parameter. In no
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33

Safdar, Faiza, and Nashva Khan. "Parental Psychological Control and Aggression Among Adolescents: Mediating Role of Emotional Dysregulation." Pakistan Journal of Psychological Research 34, no. 3 (2019): 547–64. http://dx.doi.org/10.33824/pjpr.2019.34.3.30.

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The present research examined the relationship between parental psychological control, emotional dysregulation, and aggression among adolescents. It was also intended to determine the mediating role of emotional dysregulation in the relationship between parental psychological control and aggression. It was a correlational study and purposive sample of 350 (n = 176 girls, n = 174 boys) students from school and college aged between 13 to 18 years (M = 15.77; SD = 1.37) were included in the present study. Dependency Oriented and Achievement Oriented Psychological Control Scales (Soenens, Vansteen
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34

Chaname, Julio, and Andrew Gould. "Disk and Halo Wide Binaries from the Revised Luyten Catalog: Probes of Star Formation and MACHO Dark Matter." Astrophysical Journal 601, no. 1 (2004): 289–310. http://dx.doi.org/10.1086/380442.

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35

De Bari, Cosimo, Francesco Dell'Accio, Frank Vandenabeele, Joris R. Vermeesch, Jean-Marc Raymackers, and Frank P. Luyten. "Skeletal muscle repair by adult human mesenchymal stem cells from synovial membrane." Journal of Cell Biology 160, no. 6 (2003): 909–18. http://dx.doi.org/10.1083/jcb.200212064.

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We have demonstrated previously that adult human synovial membrane-derived mesenchymal stem cells (hSM-MSCs) have myogenic potential in vitro (De Bari, C., F. Dell'Accio, P. Tylzanowski, and F.P. Luyten. 2001. Arthritis Rheum. 44:1928–1942). In the present study, we have characterized their myogenic differentiation in a nude mouse model of skeletal muscle regeneration and provide proof of principle of their potential use for muscle repair in the mdx mouse model of Duchenne muscular dystrophy. When implanted into regenerating nude mouse muscle, hSM-MSCs contributed to myofibers and to long term
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36

Hintzen, Paul, Terry D. Oswalt, James Liebert, and Edward M. Sion. "Three very cool degenerate stars in Luyten common proper motion binaries - Implications for the age of the galactic disk." Astrophysical Journal 346 (November 1989): 454. http://dx.doi.org/10.1086/168025.

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37

Wroblewski, H., and E. Costa. "Proper motions of Luyten Catalogue stars with declinations between -5° and -30° and right ascensions between 13h 30m and 24h." Astronomy and Astrophysics Supplement Series 142, no. 3 (2000): 369–71. http://dx.doi.org/10.1051/aas:2000157.

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38

Oswalt, Terry D., Paul M. Hintzen, and Willem J. Luyten. "Identifications and limited spectroscopy for Luyten common proper motion stars with probable white dwarf components. I - Pair brighter than 17th magnitude." Astrophysical Journal Supplement Series 66 (April 1988): 391. http://dx.doi.org/10.1086/191263.

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39

An Koning, Yo. "Theo Ingenhoven, Ariëtte van Reekum, Bert van Luyn & Patrick Luyten (red.) (2012). Handboek borderline persoonlijkheidsstoornis.Utrecht: de Tijdstroom, 554 pp., € 49,-." Tijdschrift voor Psychotherapie 39, no. 1 (2013): 58–62. http://dx.doi.org/10.1007/s12485-013-0010-z.

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40

Santos, Victor João da Rocha Maia, and Rosane Nunes Garcia. "HISTÓRIAS EM QUADRINHOS: BREVE HISTÓRICO, CONCEITOS E UTILIZAÇÃO NO ENSINO DAS CIÊNCIAS DA NATUREZA." Cadernos de Educação Tecnologia e Sociedade 12, no. 2 (2019): 90. http://dx.doi.org/10.14571/brajets.v12.n2.90-100.

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Comics have always been and will always be a mass medium whose focus is entertainment; however, as a type of language, its use and adaptation for the educational environment is relatively recent. In the 1980s in Brazil textbooks started to display some comics. Nonetheless, only in 1997, with the creation of PCNs, were comics officially incorporated in the classroom pedagogical praxis. The term “comic strips” and its many variations have mainly negative connotations, which have persisted until now and which have impacted the potential of this type of language in Education. Nevertheless, Brazili
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Araújo, Valéria Alves de, and Aurelania Maria De Carvalho Menezes. "Histórias em Quadrinhos: A Importância do Gênero no Processo de Alfabetização / Comics: The Importance of Gender in the Literacy Process." ID on line REVISTA DE PSICOLOGIA 14, no. 53 (2020): 867–77. http://dx.doi.org/10.14295/idonline.v14i53.2921.

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Resumo: Este trabalho trouxe as Histórias em Quadrinhos, também conhecidas como HQs, como o foco principal, tendo em vista que há muito tempo vem divertindo e ensinando pessoas no mundo inteiro. Elas têm a capacidade de levar informações e com isso, promover o conhecimento, pois por tal capacidade, nos dias atuais, as escolas têm utilizado as quadrinhas como recursos metodológicos. As Histórias em Quadrinhos possuem uma linguagem única, ou seja, universal, que se atualiza a cada geração, sempre proporcionando o desenvolvimento da criticidade. A pesquisa buscou compreender e analisa como as his
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42

Jones, Hugh R. A. "Ground-Based Surveys For Low-Luminosity Stars." Highlights of Astronomy 11, no. 1 (1998): 421–22. http://dx.doi.org/10.1017/s1539299600021614.

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Most of what we know about the Luminosity and mass function of low-mass stars has been derived from analysis of ground-based photometric and astrometric Surveys. A major uncertainty in the Interpretation of such surveys lies in the appropriate correction for unresolved binaries and in the use of a reliable colour-magnitude relation. various new surveys are now uncovering large numbers of objects which should rapidly ameliorate these ambiguities.The recent discovery of brown dwarfs and planets has highlighted the importance of low-luminosity stars. once we understand their spectra and colours a
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43

Lauteslager, Max. "Patrick Luyten, Philippe Van Haute & Andreas De Block (red.) (2007). Psychoanalyse, cognitieve psychologie en evidence-based medicine. Leuven: LannooCampus. 144 pp., € 19,95." Tijdschrift voor Psychotherapie 35, no. 2 (2009): 143–47. http://dx.doi.org/10.1007/bf03080485.

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44

Singh, Jagadish, A. E. Perdiou, Jessica Mrumun Gyegwe та V. S. Kalantonis. "Periodic orbits around the collinear equilibrium points for binary Sirius, Procyon, Luhman 16,α-Centuari and Luyten 726-8 systems: the spatial case". Journal of Physics Communications 1, № 2 (2017): 025008. http://dx.doi.org/10.1088/2399-6528/aa8976.

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45

Kopala-Sibley, Daniel C., David C. Zuroff, Nicola Hermanto, and Keven Joyal-Desmarais. "The development of self-definition and relatedness in emerging adulthood and their role in the development of depressive symptoms." International Journal of Behavioral Development 40, no. 4 (2015): 302–12. http://dx.doi.org/10.1177/0165025415573640.

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According to Blatt (2004; Blatt & Luyten, 2009) and others (e.g., Beck, Epstein, Harrison, & Emery, 1983), establishing positive self-definition and mature relatedness to others represent core lifespan developmental tasks. In a sample of emerging adults, this study examined the effects of the quality of one close friendship and changes in romantic relationship status on the development of maladaptive personality traits from each domain (self-criticism and neediness and connectedness), and the effects of changes in these personality factors on the development of depressive symptoms. Par
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46

Wroblewski, H., and C. Torres. "New proper motion determination of Luyten catalogue stars (LTT) with declination between $-5^\circ$ and $-30^\circ$ and right ascension between 0h and 13h 30m." Astronomy and Astrophysics Supplement Series 128, no. 3 (1998): 457–58. http://dx.doi.org/10.1051/aas:1998157.

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47

Woll, Christian Franz Josef, and Felix D. Schönbrodt. "A Series of Meta-Analytic Tests of the Efficacy of Long-Term Psychoanalytic Psychotherapy." European Psychologist 25, no. 1 (2020): 51–72. http://dx.doi.org/10.1027/1016-9040/a000385.

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Abstract. Recent meta-analyses come to conflicting conclusions about the efficacy of long-term psychoanalytic psychotherapy (LTPP). Our first goal was to reproduce the most recent meta-analysis by Leichsenring, Abbass, Luyten, Hilsenroth, and Rabung (2013) who found evidence for the efficacy of LTPP in the treatment of complex mental disorders. Our replicated effect sizes were in general slightly smaller. Second, we conducted an updated meta-analysis of randomized controlled trials comparing LTPP (lasting for at least 1 year and 40 sessions) to other forms of psychotherapy in the treatment of
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Cerovečki, Ivana, and Roland de Szoeke. "How Purely Wind-Driven Long Planetary Geostrophic Waves May Be Energized in the Western Part of Ocean Subtropical Gyres." Journal of Physical Oceanography 37, no. 1 (2007): 60–70. http://dx.doi.org/10.1175/jpo2977.1.

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Abstract Satellite observations and idealized numerical studies reveal intensification of long-period (on the order of one cycle per year) waves in the western part of ocean basins. The authors explore the idea that the intensification is associated with the spatial growth of purely time periodic, but baroclinically unstable, motions. The framework is a simple idealized 2½-layer model in which only the upper layer is directly forced by the wind, a setting similar to the shadow zone of the Luyten–Pedlosky–Stommel (LPS) model. The upper two layers participate in the wave motion, which is driven
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Philips, Jennifer, and Ira Herskowitz. "Osmotic Balance Regulates Cell Fusion during Mating in Saccharomyces cerevisiae." Journal of Cell Biology 138, no. 5 (1997): 961–74. http://dx.doi.org/10.1083/jcb.138.5.961.

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Successful zygote formation during yeast mating requires cell fusion of the two haploid mating partners. To ensure that cells do not lyse as they remodel their cell wall, the fusion event is both temporally and spatially regulated: the cell wall is degraded only after cell–cell contact and only in the region of cell–cell contact. To understand how cell fusion is regulated, we identified mutants defective in cell fusion based upon their defect in mating to a fus1 fus2 strain (Chenevert, J., N. Valtz, and I. Herskowitz. 1994. Genetics 136:1287–1297). Two of these cell fusion mutants are defectiv
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Narayan, Ashutosh, and Nutan Singh. "Higher order resonance stability of triangular libration points for radiating primaries in ER3BP." International Journal of Advanced Astronomy 3, no. 1 (2015): 26. http://dx.doi.org/10.14419/ijaa.v3i1.4334.

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<p>The main aim of this paper is to study the existence of resonance and stability of the triangular equilibrium points in the framework of ER3BP when both the attracting bodies are sources of radiation at w<sub>1</sub>=w<sub>2</sub>, w<sub>1</sub>=2w<sub>2</sub>, w<sub>1</sub>=3w<sub>2</sub> in both circular and elliptical cases .A practical application of this model could be seen in the case of binary systems ( Achird, Luyten, α Cen- AB, Kruger 60, Xi Bootis). The study is carried out both analytically and numerica
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