All Relations between star and asymmetrical neuron

Publication Sentence Publish Date Extraction Date Species
Andrew Vanderburg, John Asher Johnson, Saul Rappaport, Allyson Bieryla, Jonathan Irwin, John Arban Lewis, David Kipping, Warren R Brown, Patrick Dufour, David R Ciardi, Ruth Angus, Laura Schaefer, David W Latham, David Charbonneau, Charles Beichman, Jason Eastman, Nate McCrady, Robert A Wittenmyer, Jason T Wrigh. A disintegrating minor planet transiting a white dwarf. Nature. vol 526. issue 7574. 2015-11-17. PMID:26490620. the strongest transit signals occur every 4.5 hours and exhibit varying depths (blocking up to 40 per cent of the star's brightness) and asymmetric profiles, indicative of a small object with a cometary tail of dusty effluent material. 2015-11-17 2023-08-13 Not clear
L Adamczyk, J K Adkins, G Agakishiev, M M Aggarwal, Z Ahammed, I Alekseev, J Alford, A Aparin, D Arkhipkin, E C Aschenauer, G S Averichev, A Banerjee, R Bellwied, A Bhasin, A K Bhati, P Bhattarai, J Bielcik, J Bielcikova, L C Bland, I G Bordyuzhin, J Bouchet, A V Brandin, I Bunzarov, T P Burton, J Butterworth, H Caines, M Calderón de la Barca Sánchez, J M Campbell, D Cebra, M C Cervantes, I Chakaberia, P Chaloupka, Z Chang, S Chattopadhyay, J H Chen, X Chen, J Cheng, M Cherney, W Christie, G Contin, H J Crawford, S Das, L C De Silva, R R Debbe, T G Dedovich, J Deng, A A Derevschikov, B di Ruzza, L Didenko, C Dilks, X Dong, J L Drachenberg, J E Draper, C M Du, L E Dunkelberger, J C Dunlop, L G Efimov, J Engelage, G Eppley, R Esha, O Evdokimov, O Eyser, R Fatemi, S Fazio, P Federic, J Fedorisin, Z Feng, P Filip, Y Fisyak, C E Flores, L Fulek, C A Gagliardi, D Garand, F Geurts, A Gibson, M Girard, L Greiner, D Grosnick, D S Gunarathne, Y Guo, S Gupta, A Gupta, W Guryn, A Hamad, A Hamed, R Haque, J W Harris, L He, S Heppelmann, S Heppelmann, A Hirsch, G W Hoffmann, D J Hofman, S Horvat, H Z Huang, B Huang, X Huang, P Huck, T J Humanic, G Igo, W W Jacobs, H Jang, K Jiang, E G Judd, S Kabana, D Kalinkin, K Kang, K Kauder, H W Ke, D Keane, A Kechechyan, Z H Khan, D P Kikola, I Kisel, A Kisiel, D D Koetke, T Kollegger, L K Kosarzewski, L Kotchenda, A F Kraishan, P Kravtsov, K Krueger, I Kulakov, L Kumar, R A Kycia, M A C Lamont, J M Landgraf, K D Landry, J Lauret, A Lebedev, R Lednicky, J H Lee, W Li, Y Li, C Li, N Li, Z M Li, X Li, X Li, M A Lisa, F Liu, T Ljubicic, W J Llope, M Lomnitz, R S Longacre, X Luo, L Ma, R Ma, Y G Ma, G L Ma, N Magdy, R Majka, A Manion, S Margetis, C Markert, H Masui, H S Matis, D McDonald, K Meehan, N G Minaev, S Mioduszewski, B Mohanty, M M Mondal, D A Morozov, M K Mustafa, B K Nandi, Md Nasim, T K Nayak, G Nigmatkulov, L V Nogach, S Y Noh, J Novak, S B Nurushev, G Odyniec, A Ogawa, K Oh, V Okorokov, D L Olvitt, B S Page, R Pak, Y X Pan, Y Pandit, Y Panebratsev, B Pawlik, H Pei, C Perkins, A Peterson, P Pile, M Planinic, J Pluta, N Poljak, K Poniatowska, J Porter, M Posik, A M Poskanzer, N K Pruthi, J Putschke, H Qiu, A Quintero, S Ramachandran, S Raniwala, R Raniwala, R L Ray, H G Ritter, J B Roberts, O V Rogachevskiy, J L Romero, A Roy, L Ruan, J Rusnak, O Rusnakova, N R Sahoo, P K Sahu, I Sakrejda, S Salur, J Sandweiss, A Sarkar, J Schambach, R P Scharenberg, A M Schmah, W B Schmidke, N Schmitz, J Seger, P Seyboth, N Shah, E Shahaliev, P V Shanmuganathan, M Shao, B Sharma, M K Sharma, W Q Shen, S S Shi, Q Y Shou, E P Sichtermann, R Sikora, M Simko, M J Skoby, D Smirnov, N Smirnov, L Song, P Sorensen, H M Spinka, B Srivastava, T D S Stanislaus, M Stepanov, R Stock, M Strikhanov, B Stringfellow, M Sumbera, B J Summa, X Sun, X M Sun, Z Sun, Y Sun, B Surrow, D N Svirida, M A Szelezniak, Z Tang, A H Tang, T Tarnowsky, A N Tawfik, J H Thomas, A R Timmins, D Tlusty, M Tokarev, S Trentalange, R E Tribble, P Tribedy, S K Tripathy, B A Trzeciak, O D Tsai, T Ullrich, D G Underwood, I Upsal, G Van Buren, G van Nieuwenhuizen, M Vandenbroucke, R Varma, A N Vasiliev, R Vertesi, F Videbaek, Y P Viyogi, S Vokal, S A Voloshin, A Vossen, F Wang, Y Wang, H Wang, J S Wang, Y Wang, G Wang, G Webb, J C Webb, L Wen, G D Westfall, H Wieman, S W Wissink, R Witt, Y F Wu, Z Xiao, W Xie, K Xin, Y F Xu, N Xu, Z Xu, Q H Xu, H Xu, Y Yang, Y Yang, C Yang, S Yang, Q Yang, Z Ye, P Yepes, L Yi, K Yip, I-K Yoo, N Yu, H Zbroszczyk, W Zha, X P Zhang, J B Zhang, J Zhang, Z Zhang, S Zhang, Y Zhang, J L Zhang, F Zhao, J Zhao, C Zhong, L Zhou, X Zhu, Y Zoulkarneeva, M Zyza. Observation of Charge Asymmetry Dependence of Pion Elliptic Flow and the Possible Chiral Magnetic Wave in Heavy-Ion Collisions. Physical review letters. vol 114. issue 25. 2015-09-28. PMID:26197122. we present measurements of π(-) and π(+) elliptic flow, v(2), at midrapidity in au+au collisions at √[s(nn)]=200, 62.4, 39, 27, 19.6, 11.5, and 7.7 gev, as a function of event-by-event charge asymmetry, a(ch), based on data from the star experiment at rhic. 2015-09-28 2023-08-13 Not clear
Weichao Shi, Andrew L Hamilton, Kris T Delaney, Glenn H Fredrickson, Edward J Kramer, Christos Ntaras, Apostolos Avgeropoulos, Nathaniel A Lyn. Creating Extremely Asymmetric Lamellar Structures via Fluctuation-Assisted Unbinding of Miktoarm Star Block Copolymer Alloys. Journal of the American Chemical Society. vol 137. issue 19. 2015-07-20. PMID:25915769. creating extremely asymmetric lamellar structures via fluctuation-assisted unbinding of miktoarm star block copolymer alloys. 2015-07-20 2023-08-13 Not clear
Weichao Shi, Andrew L Hamilton, Kris T Delaney, Glenn H Fredrickson, Edward J Kramer, Christos Ntaras, Apostolos Avgeropoulos, Nathaniel A Lyn. Creating Extremely Asymmetric Lamellar Structures via Fluctuation-Assisted Unbinding of Miktoarm Star Block Copolymer Alloys. Journal of the American Chemical Society. vol 137. issue 19. 2015-07-20. PMID:25915769. we report the creation of highly asymmetric lamellar structures with a well-designed miktoarm star block copolymer of the s(is')3 type, where s and s' are polystyrenes of different lengths and i is poly(isoprene). 2015-07-20 2023-08-13 Not clear
Galina P Demyanenko, Vishwa Mohan, Xuying Zhang, Leann H Brennaman, Katherine E S Dharbal, Tracy S Tran, Paul B Manis, Patricia F Manes. Neural cell adhesion molecule NrCAM regulates Semaphorin 3F-induced dendritic spine remodeling. The Journal of neuroscience : the official journal of the Society for Neuroscience. vol 34. issue 34. 2014-12-22. PMID:25143608. nrcam deletion in mice resulted in elevated spine densities on apical dendrites of star pyramidal cells at both postnatal and adult stages, and electron microscopy revealed increased numbers of asymmetric synapses in layer 4 of v1. 2014-12-22 2023-08-13 mouse
Laura Shin. The impact of star physicians on diffusion of a medical technology: the case of laparoscopic gastric bypass surgery. Journal of health care finance. vol 40. issue 3. 2014-10-27. PMID:25223160. at the physician level, the empirical results indicate that star physicians exert positive asymmetric influence on the adoption and utilization rates of nonstars at the same hospital. 2014-10-27 2023-08-13 Not clear
W R F Dent, M C Wyatt, A Roberge, J-C Augereau, S Casassus, S Corder, J S Greaves, I de Gregorio-Monsalvo, A Hales, A P Jackson, A Meredith Hughes, A-M Lagrange, B Matthews, D Wilne. Molecular gas clumps from the destruction of icy bodies in the β Pictoris debris disk. Science (New York, N.Y.). vol 343. issue 6178. 2014-04-10. PMID:24603151. the gas distribution is highly asymmetric, with 30% found in a single clump 85 astronomical units from the star, in a plane closely aligned with the orbit of the inner planet, β pictoris b. 2014-04-10 2023-08-12 Not clear
H H Witte, V Kulic. Branching elements for optical data buses. Applied optics. vol 20. issue 4. 2012-10-02. PMID:20309183. asymmetric 4-port couplers and star couplers with 60 ports for multimode fibers are described. 2012-10-02 2023-08-12 Not clear
Brian G Alberding, Malcolm H Chisholm, Terry L Gustafso. Detection of the singlet and triplet MM δδ* states in quadruply bonded dimetal tetracarboxylates (M = Mo, W) by time-resolved infrared spectroscopy. Inorganic chemistry. vol 51. issue 1. 2012-04-24. PMID:22129155. in the region from 1500 to 1600 cm(-1), a long-lived excited state (>2 ns) has been detected for the compounds m(2)(o(2)c(t)bu)(4) and mo(2)(o(2)c-c(6)h(5))(4) with an ir absorption at ~1540 cm(-1) assignable to the asymmetric co(2) stretch, ν(as)(co(2)), of the triplet metal-metal δ-δ star ((3)mm δδ*) state. 2012-04-24 2023-08-12 Not clear
Chris Kouvaris, Peter Tinyako. Excluding light asymmetric bosonic dark matter. Physical review letters. vol 107. issue 9. 2012-04-18. PMID:21929221. we argue that current neutron star observations exclude asymmetric bosonic noninteracting dark matter in the range from 2 kev to 16 gev, including the 5-15 gev range favored by dama and cogent. 2012-04-18 2023-08-12 Not clear
John L Hal. Learning from the time and length redefinitions, and the metre demotion. Philosophical transactions. Series A, Mathematical, physical, and engineering sciences. vol 369. issue 1953. 2011-11-15. PMID:21930567. such progress stimulates a new satellite experiment, the star mission (space-time asymmetry research). 2011-11-15 2023-08-12 Not clear
Yuichi Masubuchi, Takatoshi Yaoita, Yumi Matsumiya, Hiroshi Watanab. Primitive chain network simulations for asymmetric star polymers. The Journal of chemical physics. vol 134. issue 19. 2011-09-30. PMID:21599086. primitive chain network simulations for asymmetric star polymers. 2011-09-30 2023-08-12 Not clear
Yuichi Masubuchi, Takatoshi Yaoita, Yumi Matsumiya, Hiroshi Watanab. Primitive chain network simulations for asymmetric star polymers. The Journal of chemical physics. vol 134. issue 19. 2011-09-30. PMID:21599086. the simulations considering the fluctuation and the hopping of the branch point described well the viscoelastic data for symmetric and asymmetric star polymers with a parameter set common to the linear polymer. 2011-09-30 2023-08-12 Not clear
Yuichi Masubuchi, Takatoshi Yaoita, Yumi Matsumiya, Hiroshi Watanab. Primitive chain network simulations for asymmetric star polymers. The Journal of chemical physics. vol 134. issue 19. 2011-09-30. PMID:21599086. on the other hand, the simulations without the branch point motion predicted unreasonably slow relaxation for asymmetric star polymers. 2011-09-30 2023-08-12 Not clear
Yuichi Masubuchi, Takatoshi Yaoita, Yumi Matsumiya, Hiroshi Watanab. Primitive chain network simulations for asymmetric star polymers. The Journal of chemical physics. vol 134. issue 19. 2011-09-30. PMID:21599086. for asymmetric star polymers, further tests with and without the branch point hopping revealed that the hopping is much less important compared to the branch point fluctuation when the lengths of the short and long backbone arms are not very different and the waiting time for the branch point hopping (time for removal of all sliplinks on the short arm) is larger than the backbone relaxation time. 2011-09-30 2023-08-12 Not clear
J H Schmitt, M Kürste. A Spatially Resolved X-ray Image of a Star Like the Sun. Science (New York, N.Y.). vol 262. issue 5131. 2010-07-02. PMID:17841866. the x-ray eclipse ingress and egress are highly asymmetric compared with the optical eclipse, indicating a highly asymmetric x-ray intensity distribution on the surface of the g star. 2010-07-02 2023-08-12 Not clear
Juntao Luo, Guillaume Giguère, X X Zh. Asymmetric poly(ethylene glycol) star polymers with a cholic acid core and their aggregation properties. Biomacromolecules. vol 10. issue 4. 2010-02-01. PMID:19281151. asymmetric poly(ethylene glycol) star polymers with a cholic acid core and their aggregation properties. 2010-02-01 2023-08-12 Not clear
Juntao Luo, Guillaume Giguère, X X Zh. Asymmetric poly(ethylene glycol) star polymers with a cholic acid core and their aggregation properties. Biomacromolecules. vol 10. issue 4. 2010-02-01. PMID:19281151. the asymmetric star polymers were found to aggregate differently from cholic acid salt. 2010-02-01 2023-08-12 Not clear
Zhibin Jiang, Rong Wang, Gi Xu. Morphology and phase diagram of comb block copolymer Am+1(BC)m. The journal of physical chemistry. B. vol 113. issue 21. 2009-09-14. PMID:19422259. due to the asymmetric topology of comb copolymer am+1(bc)m, the phases and the diagrams are very different from linear abc triblock copolymer or star abc triblock copolymer. 2009-09-14 2023-08-12 Not clear
C J Horowitz, O L Caballero, D K Berr. Thermal conductivity and phase separation of the crust of accreting neutron stars. Physical review. E, Statistical, nonlinear, and soft matter physics. vol 79. issue 2 Pt 2. 2009-09-11. PMID:19391802. this could lead to an asymmetric star with a quadrupole deformation. 2009-09-11 2023-08-12 Not clear