Results 1 to 10 of about 82,917 (97)

The Citation Impact of Digital Preprint Archives for Solar Physics Papers [PDF]

, 2006
Papers that are posted to a digital preprint archive are typically cited twice as often as papers that are not posted. This has been demonstrated for papers published in a wide variety of journals, and in many different subfields of astronomy.
Metcalfe, Travis S.
core   +5 more sources

Dynamical Interactions and the Black Hole Merger Rate of the Universe [PDF]

, 2007
Binary black holes can form efficiently in dense young stellar clusters, such as the progenitors of globular clusters, via a combination of gravitational segregation and cluster evaporation.
Frederic A. Rasio, M. Freitag, N. Bastian, Richard O’Shaughnessy, Ryan M. O’Leary, S. F. Portegies Zwart, T. M. Heckman   +6 more
core   +2 more sources

Deep I-band Imaging of z=5.99 Quasar

, 2002
Deep I-band imaging was carried out to search for the optical counterpart of the X-ray jet candidate near SDSS 1306+0356, reported by Schwartz (2002, astro-ph/0202190).
Ivanov, Valentin D.
core   +1 more source

E-prints and Journal Articles in Astronomy: a Productive Co-existence

, 2006
Are the e-prints (electronic preprints) from the arXiv repository being used instead of the journal articles? In this paper we show that the e-prints have not undermined the usage of journal papers in the astrophysics community.
Accomazzi, Alberto, Bohlen, Elizabeth, Eichhorn, Guenther, Ginsparg, Paul, Grant, Carolyn S., Henneken, Edwin A., Kurtz, Michael J., Murray, Stephen S., Thompson, Donna, Warner, Simeon   +9 more
core   +1 more source

Foundations of Black Hole Accretion Disk Theory [PDF]

, 2013
This review covers the main aspects of black hole accretion disk theory. We begin with the view that one of the main goals of the theory is to better understand the nature of black holes themselves.
A Brandenburg, A Ciesielski, A Kovetz, A Soltan, A Sądowski, A Sądowski, A Sądowski, A Tchekhovskoy, A Tchekhovskoy, AA Esin, AA Esin, AA Esin, AA Esin, AC Fabian, AE Broderick, AE Broderick, AK Harding, AK Kulkarni, AM Beloborodov, AM Beloborodov, AP Lightman, AR King, AR King, B Giacomazzo, B Mashhoon, B Muchotrzeb, B Mukhopadhyay, B Paczyński, B Paczyński, B Paczyński, B Punsly, BD Farris, BJ Carr, BT Ferreira, C Done, C Done, C Roedig, CA Perez, CD Levermore, CF Gammie, CF Gammie, CF Gammie, CS Reynolds, CS Reynolds, CW Misner, D Barret, D Barret, D Barret, D Eichler, D MacDonald, D Merritt, D Proga, D Proga, D Psaltis, DE Harris, DL Meier, DM Rothstein, DN Page, EJM Colbert, EP Velikhov, ES Phinney, F Daigne, F Eisenhauer, F Melia, F Yuan, F Yuan, F Yuan, F Yuan, FE Barrio, FH Seguin, G Lesur, G Török, GI Ogilvie, GS Bisnovatyi-Kogan, H Bondi, H Riffert, HC Spruit, I Hubeny, ID Novikov, IF Mirabel, IF Mirabel, IF Mirabel, IV Artemova, IV Igumenshchev, IV Igumenshchev, IV Igumenshchev, IV Igumenshchev, J Dexter, J Frank, J Horák, J Horák, J Kormendy, J Shi, J Wilms, J-L Tassoul, J-P Lasota, J-P Lasota, J-P Lasota, J-P Lasota, J-P Villiers De, J-P Villiers De, J-P Villiers De, J-P Villiers De, J-P Villiers De, JA Font, JC Dolence, JC McKinney, JC McKinney, JC McKinney, JC McKinney, JC McKinney, JCB Papaloizou, JD Schnittman, JE Goldston, JE McClintock, JE McClintock, JE McClintock, JE Pringle, JF Hawley, JF Hawley, JF Hawley, JF Hawley, JF Hawley, JF Hawley, JF Hawley, JF Hawley, JF Hawley, JF Hawley, JF Hawley, JF Steiner, JF Steiner, JH Krolik, JH Krolik, JH Krolik, JM Bardeen, JM Bardeen, JM Bardeen, JM Miller, JM Miller, JM Miller, JM Miller, JM Miller, JM Stone, JR Wilson, JR Wilson, JR Wilson, K Kiuchi, K Makishima, K Menou, K Nobuta, K Ohsuga, K Ohsuga, K Shibata, K Shibata, KB Henisey, L Antón, L Baiotti, L Qian, L Rezzolla, L Rezzolla, L Stella, L Zanna Del, L-X Li, LD Landau, LG Fishbone, M Anderson, M Bañados, M Bejger, M Bursa, M Georganopoulos, M Jaroszyński, M Klis van der, M Kozłowski, M Machida, M Middleton, M Mościbrodzka, M Ortega-Rodríguez, M Shibata, M Sikora, MA Abramowicz, MA Abramowicz, MA Abramowicz, MA Abramowicz, MA Abramowicz, MA Abramowicz, MA Abramowicz, MA Abramowicz, MA Abramowicz, MA Abramowicz, MA Abramowicz, MA Abramowicz, MA Abramowicz, MC Begelman, MC Begelman, MC Begelman, MC Miller, MD Duez, MJ Rees, MR Garcia, N Arkani-Hamed, N Shibazaki, NI Shakura, NI Shakura, NJ Turner, O Korobkin, O Semerák, O Straub, O Straub, O Zanotti, O Zanotti, O Zanotti, OM Blaes, OM Blaes, OM Blaes, OM Blaes, P Amsterdamski, P Anninos, P Anninos, P Arras, P Ghosh, P Madau, P Rebusco, P Sharma, PAG Scheuer, PC Fragile, PC Fragile, PC Fragile, PC Fragile, PC Joss, PJ Montero, PJ Montero, R Narayan, R Narayan, R Narayan, R Narayan, R Narayan, R Narayan, R Narayan, R Narayan, R Narayan, R Narayan, R Narayan, R Narayan, R Penrose, R Penrose, R Shafee, R Shafee, R Svensson, R Takahashi, RA Araya-Góchez, RA Remillard, RA Remillard, RD Blandford, RD Blandford, RD Blandford, RE Taam, RF Penna, RF Penna, RH Boyer, RM Wald, RP Fender, RP Fender, RP Fender, RV Wagoner, RV Wagoner, RV Wagoner, S Chandrasekhar, S Gillessen, S Hirose, S Hirose, S Ichimaru, S Kato, S Koide, S Koide, S Kumar, S Rawlings, S Stepney, SA Balbus, SA Balbus, SA Balbus, SA Farrell, SC Noble, SC Noble, SE Woosley, SH Lubow, SI Raimundo, SK Chakrabarti, SL Shapiro, SM Wagh, SS Doeleman, SS Komissarov, SS Komissarov, SS Komissarov, SS Komissarov, SS Komissarov, SW Davis, SW Davis, SW Davis, T Damour, T Johannsen, T Piran, T Piran, T Sano, T Sano, T Shimura, V Karas, W Cui, X Chen, Y Kato, Y Kato, Y Zhu, ZB Etienne   +311 more
core   +3 more sources

Constraining the neutron star equation of state using Pulse Profile Modeling [PDF]

, 2019
One very promising technique for measuring the dense matter Equation of State exploits hotspots that form on the neutron star surface due to the pulsar mechanism, accretion streams, or during thermonuclear explosions in the neutron star ocean.
Watts, Anna L.
core   +3 more sources

Implementation of the trigger algorithm for the NEMO project [PDF]

, 2007
We describe the implementation of trigger algorithm specifically tailored on the characteristics of the neutrino telescope NEMO. Extensive testing against realistic simulations shows that, by making use of the uncorrelated nature of the noise produced ...
Brescia, M., d'Angelo, G., Riccio, G.
core   +1 more source

Planetary Collisions: Electromagnetic Signals

, 2003
We investigate the electromagnetic signals accompanied with planetary collisions and their event rate, and explore the possibility of directly detecting such events.
Sigurdsson, Steinn, Zhang, Bing
core   +1 more source

Primordial Nucleosynthesis with CMB Inputs: Probing the Early Universe and Light Element Astrophysics [PDF]

, 2001
Cosmic microwave background (CMB) determinations of the baryon-to-photon ratio $\eta \propto \Omega_{\rm baryon} h^2$ will remove the last free parameter from (standard) big bang nucleosynthesis (BBN) calculations. This will make BBN a much sharper probe
Balbi, Barriga, Bartlett, Birkel, Bond, Bonifacio, Brian D. Fields, Burles, Cardall, Copi, Cyburt, de Bernardis, Ellis, Epstein, Fields, Fields, Fiorentini, Groom, Hannestad, Hata, Izotov, Jaffe, Jedamzik, Jungman, Jungman, Kaplinghat, Keith A. Olive, Kernan, Kurki-Suonio, Lisi, Malaney, O'Meara, Olive, Olive, Olive, Olive, Padin, Peimbert, Richard H. Cyburt, Ryan, Ryan, Sarkar, Scherrer, Schneider, Schramm, Steigman, Tegmark, Walker, Zaldarriaga   +48 more
core   +3 more sources

Statistical analysis of the trigger algorithm for the NEMO project [PDF]

, 2007
We discuss the performances of a trigger implemented for the planned neutrino telescope NEMO. This trigger seems capable to discriminate between the signal and the strong background introduced by atmospheric muons and by the beta decay of the K-40 nuclei
Brescia, M., D'Angelo, G., Riccio, G.
core   +1 more source