Results 11 to 20 of about 801,794 (331)
Participação das mulheres na graduação da Faculdade de Odontologia da Universidade Federal do Rio Grande do Sul
Revista da Faculdade de Odontologia de Porto Alegre, 2010 Em 1866, na Universidade de Ohio, graduou-se a primeira mulher da história da Odontologia, sendo que a inserção da mulher na Odontologia ocorreu de forma lenta e gradual, acompanhando o desenvolvimento histórico e cultural da sociedade. Um dos fatores que faz com que a mulher opte pela carreira odontológica é o fato de poder exercer o trabalho de forma Baldissera, Renata Dos Santos, Grecca, Fabiana Soares, dos Santos, Régis Burmeister +2 moreopenaire +8 more sourcesOn the Use of Field RR Lyrae as Galactic Probes. V. Optical and Radial Velocity Curve Templates [PDF]
Astrophysical Journal, 2021 We collected the largest spectroscopic catalog of RR Lyrae (RRLs) including ≈20,000 high-, medium-, and low-resolution spectra for ≈10,000 RRLs. We provide the analytical forms of radial velocity curve (RVC) templates.V. Braga, J. Crestani, M. Fabrizio, G. Bono, G. Preston, C. Sneden, J. Storm, S. Kamann, M. Latour, H. Lala, B. Lemasle, Z. Prudil, G. Altavilla, B. Chaboyer, M. Dall’ora, I. Ferraro, C. Gilligan, G. Fiorentino, G. Iannicola, L. Inno, S. Kwak, M. Marengo, S. Marinoni, P. Marrese, C. Martínez-Vázquez, M. Monelli, J. Mullen, N. Matsunaga, J. Neeley, P. Stetson, E. Valenti, M. T. I. A. D. Roma, M. Catone, Italy., S. Center, Roma, D. D. Astronomia, Universidade Federal do Rio Grande do Sul, P. Alegre, Brazil, D. Fisica, Universita' di Roma Tor Vergata, The Observatories of the Carnegie Institution for Science, Pasadena, Ca, Usa, D. O. Astronomy, M. Observatory, The University of Texas, Austin, Tx, L. I. A. Potsdam, Potsdam, H Germany, A. R. Institute, Liverpool John Moore's University, Liverpool, UK., Institute for Computational Astrophysics, Georg-August-Universitat Gottingen, A. Rechen-Institut, Zentrum fur Astronomie der Universitat Heidelberg, Heidelberg, Universit'e de Nice Sophia-antipolis, Cnrs, Observatoire Cote d'Azur, Laboratoire Lagrange, Nice, France, D. Physics, Astronomy, Dartmouth College, Hanover, I. -. Capodimonte, Napoli, Universita degli Studi di NapoliParthenope'', I. S. University, Ames, Ia, Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, L. Serena, Chile., Instituto de Astrof'isica de Canarias, La Laguna, Tenerife, Spain., T. U. O. Tokyo, Tokyo, Japan., Florida Atlantic University, Boca Raton, Fl, H. Astronomy, Astrophysics, National Research Council, Victoria, bc, Canada, E. Observatory, G. B. Munchen, Instituto Milenio de Astrof'isica, Santiago, P. U. C. D. Chile, Instituto de Astrofisica +104 moresemanticscholar +1 more sourceOn the Use of Field RR Lyrae as Galactic Probes. II. A New ΔS Calibration to Estimate Their Metallicity [PDF]
Astrophysical Journal, 2020 We performed the largest and most homogeneous spectroscopic survey of field RR Lyraes (RRLs). We secured ≈6300 high-resolution (HR, R ∼ 35,000) spectra for 143 RRLs (111 fundamental, RRab; 32 first-overtone, RRc).J. Crestani, M. Fabrizio, V. Braga, C. Sneden, G. Preston, I. Ferraro, G. Iannicola, G. Bono, A. Alves-Brito, M. Nonino, V. D’Orazi, L. Inno, M. Monelli, J. Storm, G. Altavilla, B. Chaboyer, M. Dall’ora, G. Fiorentino, C. Gilligan, E. Grebel, H. Lala, B. Lemasle, M. Marengo, S. Marinoni, P. Marrese, C. Martínez-Vázquez, N. Matsunaga, J. Mullen, J. Neeley, Z. Prudil, R. Silva, P. Stetson, F. Thévenin, E. Valenti, A. Walker, M. Z. D. D. Astronomia, Universidade Federal do Rio Grande do Sul, P. Alegre, Brazil, D. Fisica, Universita' di Roma Tor Vergata, Roma, Italy., I. Roma, M. Catone, S. Center, D. O. Astronomy, M. Observatory, The University of Texas, Austin, Tx, Usa, The Observatories of the Carnegie Institution for Science, Pasadena, Ca, Inaf Trieste, Trieste, Inaf - Padova, Padova, S. O. Physics, Astronomy, M. University, Clayton, Melbourne, Australia., Universita degli Studi di NapoliParthenope'', Napoli, Instituto de Astrof'isica de Canarias, La Laguna, Tenerife, Spain., L. I. A. Potsdam, Potsdam, H Germany, D. Physics, Dartmouth College, Hanover, I. -. Capodimonte, Universit'e de Nice Sophia-antipolis, Cnrs, Observatoire Cote d'Azur, Laboratoire Lagrange, Nice, France, A. Rechen-Institut, Zentrum fur Astronomie der Universitat Heidelberg, Heidelberg, I. S. University, Ames, Ia, Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, L. Serena, Chile., T. U. O. Tokyo, Tokyo, Japan., Florida Atlantic University, Boca Raton, Fl, H. Astronomy, Astrophysics, National Research Council, Victoria, bc, Canada, E. Observatory, G. B. Munchen, Instituto Milenio de Astrof'isica, Santiago, P. U. C. D. Chile, Instituto de Astrofisica +111 moresemanticscholar +1 more sourceThe statistics of lambda CDM Halo Concentrations [PDF]
, 2007 We use the Millennium Simulation (MS) to study the statistics of Λ cold dark matter (ΛCDM) halo concentrations at z= 0. Our results confirm that the average halo concentration declines monotonically with mass; the concentration–mass relation is well ...A. F. Neto, Liang Gao, P. Bett, S. Cole, J. Navarro, C. Frenk, S. White, V. Springel, A. V. I. D. F'isica, Universidade Federal do Rio Grande do Sul, RS PortoAlegre, Brazil Institute of Cosmology, D. Physics, U. Durham, Durham, U. D. O. Physics, Astronomy, U. Victoria, Victoria, Canada Max-Planck Institute for Astrophysics, Garching, H Germany +21 moresemanticscholar +1 more sourceCHEERS Results from NGC 3393. III. Chandra X-Ray Spectroscopy of the Narrow Line Region [PDF]
Astrophysical Journal, 2018 We present spatially resolved Chandra narrow-band imaging and imaging spectroscopy of NGC 3393. This galaxy hosts a Compton-thick Seyfert 2 active galactic nucleus (AGN) with sub-kpc bipolar outflows that are strongly interacting with the circumnuclear ...W. Maksym, G. Fabbiano, M. Elvis, M. Karovska, A. Paggi, J. Raymond, Junfeng Wang, T. Storchi-Bergmann, Guido Risaliti Harvard-Smithsonian Center for Astrophysics, U. Torino, Istituto Nazionale Fisica Nucleare, I. Torino, Xiamen University, Universidade Federal do Rio Grande do Sul, INAF-Arcetri Observatory +14 moresemanticscholar +1 more sourceThe first spectroscopic dust reverberation programme on active galactic nuclei: the torus in NGC 5548 [PDF]
Monthly notices of the Royal Astronomical Society, 2019
We have recently initiated the first spectroscopic dust reverberation programme on active galactic nuclei in the near-infrared. Spectroscopy enables measurement of dust properties, such as flux, temperature, and covering factor, with higher precision ...H. Landt, M. Ward, D. Kynoch, C. Packham, G. Ferland, A. Lawrence, J. Pott, J. Esser, K. Horne, D. Starkey, D. Malhotra, M. Fausnaugh, B. Peterson, R. Wilman, R. Riffel, T. Storchi-Bergmann, A. Barth, C. Villforth, H. University, University of Texas at San Antonio, Naoj, U. Kentucky, U. Edinburgh, MPIfA, U. S. Andrews, U. I. Urbana-Champaign, Mit, The Ohio State University, Ccapp, Stsci, Universidade Federal de Santa Maria, Universidade Federal do Rio Grande do Sul, U. California, Irvine, U. Bath, University of Johannesburg +35 moresemanticscholar +1 more source