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3por Rhee, George“…The visible universe consists of stars and galaxies. One of the challenges of astronomy is to understand how galaxies and stars first came into existence over thirteen billion years ago. …”
Publicado 2013
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5por Karaparambil, Vivek Chandran, Manjarekar, Narayan Suresh, Singru, Pravin Madanrao“…The localization of the center of the star image formed on a sensor array directly affects attitude estimation accuracy. …”
Publicado 2023
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6por Allen, Bruce“…I describe the current status of the Einstein@Home search for new neutron stars, using data from the Laser Interferometer Gravitational-wave Observatory (LIGO), from the Arecibo and Parkes radio telescopes, and from the Fermi gamma-ray satellite. …”
Publicado 2012
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7por Saraceno, Paolo“…The final part is dedicated to the search for extraterrestrial beings with identifiable life forms. …”
Publicado 2012
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14por Aglietta, M, Alpat, B, Alyea, E D, Antonioli, P, Anzivino, Giuseppina, Badino, G, Ban, Y, Bari, G, Basile, M, Benelli, A, Berezinsky, Veniamin Sergeevich, Bergamasco, L, Bianco, S, Bizzeti, A, Bruni, G, Cao, Y, Cara Romeo, G, Casaccia, R, Castagnoli, C, Castellina, A, Chen, K, Chen, R, Chinellato, J A, Cifarelli, Luisa, Cini, G, Cong, S, Contin, A, Dadikin, V L, Dardo, M, De Silva, A, Deutsch, M, Dos Santos, L G, Enikeev, R I, Fabbri, Franco Luigi, Fulgione, W, Galeotti, P, Ghia, P L, Giusti, P, Grianti, F, Gu, S, Hafen, E S, Haridas, P, Iacobucci, G, Inoue, N, Khalchukov, F F, Korolkova, E V, Kortchaguin, P V, Kortchaguin, V B, Kudryavtsev, V A, Landi, G, Lau, K, Lin, X, Lü, L, Ma, J, Ma, Z, Maccarrone, G D, Malguin, A S, Mao, Z, Markov, M A, Massam, Thomas, Mayes, B W, Mengotti-Silva, N, Misaki, A, Mo, G H, Monteleoni, B, Morello, C, Moromisato, J H, Nania, R, Navarra, G, Panaro, L, Parks, D P, Pelfer, P G, Periale, L, Picchi, P, Pinna, P, Pinsky, L, Pless, I A, Pu, M, Pyrlik, J, Qiu, J, Ryasny, V G, Ryazhskaya, O G, Saavedra, O, Saitô, K, Sanders, D, Sartorelli, G, Sarwar, S, Shen, D, Susinno, G, Talochkin, V P, Tang, H, Tang, J, Tian, W, Trinchero, G C, Turtelli, A, Uman, I, Vallania, P, Vernetto, S, von Goeler, E, Votano, L, Wada, T, Wang, F, Wang, H, Wang, S, Weathers, R, Weinstein, R, Widgoff, M, Xu, L, Xu, Z, Yakushev, V F, Yamamoto, I, Yi, G, Zallo, A, Zatsepin, G T, Zhou, X, Zhu, X, Zhuang, B, Zichichi, AntoninoEnlace del recurso
Publicado 1992
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15por Ansari, R., Auriere, M., Baillon, P., Bouquet, A., Coupinot, G., Coutures, Ch., Ghesquiere, C., Giraud-Heraud, Y., Gondolo, P., Hecquet, J., Kaplan, J., Du, Y.Le, Melchior, A.L., Moniez, M., Picat, J.P., Soucail, G.“…However most stars of M31 are not resolved and one has to use the ``pixel method'': monitor the pixels of the image rather than the stars. …”
Publicado 1996
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17“…We derive and interpret the equation of state for ADM with both attractive and repulsive interactions, and solve the Tolman-Oppenheimer-Volkoff equations to find equilibrium sequences and maximum masses of ADM stars. Gravitational wave searches can utilize our solutions to model exotic compact objects (ECOs). …”
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18“…This paper describes the multilayer voting algorithm, a novel autonomous star identification method for spacecraft attitude determination. …”
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19“…In this paper an improved brightness referenced star identification algorithm is presented. This algorithm utilizes the k-vector search theory and adds imaged stars' intensities to narrow the search scope and therefore increase the efficiency of the matching process. …”
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20por Raffelt, Georg G“…Stars are powerful sources for weakly interacting particles that are produced by nuclear or plasma processes in their hot interior. …”
Publicado 2002
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