Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Angela Krabbe"'
Autor:
Diana P. P. Andrade, Dinalva A. Sales, Carla M. Canelo, Angela Krabbe, J. A. Hernandez-Jimenez, A. Silva-Ribeiro, A. F. Monteiro
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 509:327-344
We present a study for a sample of galaxies with active nuclei to characterize the main type of PAH molecules present in these objects and the local physical conditions of their irradiating sources, as well as the characteristics of the residing ioni
Autor:
Mónica V. Cardaci, Rogemar A. Riffel, Anna Feltre, C. P. Aydar, Guillermo F. Hägele, Oli L. Dors, Mark Kojo Armah, Angela Krabbe, Rogério Riffel
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
For the first time, neon abundance has been derived in the narrow line region from a sample of Seyfert 2 nuclei. In view of this, we compiled from the literature fluxes of optical and infrared (IR) narrow emission lines for 35 Seyfert 2 nuclei in the
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 506:L11-L15
We use Gemini GMOS-IFU observations of three luminous nearby Seyfert galaxies (Mrk79, Mrk348 and Mrk607) to estimate the electron temperature ($T_{\rm e}$) fluctuations in the inner 0.4-1.1 kpc region of these galaxies. Based on $T_{\rm e}$ determina
Autor:
L. J. de Melo de Azevedo, L. Katena, Antonio Kanaan, Paula Coelho, M. V. Costa-Duarte, F. Urrutia-Viscarra, A. Schnorr Müller, Irapuan Rodrigues, Erik V.R. de Lima, Angela Krabbe, David Alexander Kann, M. Vika, Carlos Gabriel Escudero, S. Alencar, Dennis Zaritsky, Nina S. T. Hirata, G. Damke, Fernando Roig, H. Farías, Leonardo A. Almeida, Anthony H. Gonzalez, D. Brito-Silva, Favio Raúl Faifer, F. Almeida-Fernandes, Luca Izzo, H. J. Rocha Pinto, O. L. Dors, W. A. Santos, M. Jaque Arancibia, Rafael M. Santucci, Pieter Westera, Yara L. Jaffé, Bruno Quint, Kanak Saha, R. S. Nemmen, Roberto K. Saito, L. A. Gutiérrez-Soto, Silvia Rossi, Leandro Alberto Sesto, Lilianne Mariko Izuti Nakazono, Ana L. Chies-Santos, L. Azanha, C. Labayru, Christina C. Thöne, William Schoenell, C. Lima-Dias, A. de Ugarte Postigo, S. S. Eikenberry, Carlos A. Fernandes, E. A. Hartmann, R. A. Ortega-Minakata, L. Sampedro, Ramachrisna Teixeira, P. Amram, Daniela Lazzaro, N. Muñoz-Elgueta, R. Lopes de Oliveira, C. H. Veiga, E. Pattaro, Teresa Santos-Silva, C. B. Pereira, S. V. Werner, R. Cid Fernandes, F. R. Herpich, Alexandre S. Oliveira, Simone Daflon, R. S. de Souza, J. S. Alcaniz, Analia Viviana Smith Castelli, Beatriz B. Siffert, D. F. De Paula, C. Bonatto, H. D. Perottoni, Marina Trevisan, Y. Jimenez-Teja, Eduardo S. Pereira, L. Sodré, Timothy C. Beers, M. Borges Fernandes, A. Werle, M. L. Buzzo, C. Mendes de Oliveira, M. Castejon, Vinicius M. Placco, Richard L. Donnerstein, Javier Alonso-García, Roderik Overzier, S. Bonoli, J. A. Hernandez-Jimenez, C. Queiroz, Beatriz Luci Fernandes, Rodolfo H. Barbá, R. Monteiro-Oliveira, Thiago S. Gonçalves, R. Silva, Alvaro Alvarez-Candal, Arianna Cortesi, G. Fabiano de Souza, Karín Menéndez-Delmestre, Eduardo S. Cypriano, T. Ribeiro, J. Caffer, Zach Cano, Martin Makler, S. Fontes, H. S. Xavier, C. L. Barbosa, V. Jatenco-Pereira, K. G. Diem, Amanda R. Lopes, M. L. L. Dantas, R. C. Thom de Souza, A. Galarza, Jane Gregorio-Hetem, J. L. Nilo Castellón, A. Z. Vitorelli, D. Ortíz, R. de Menezes, Denise R. Gonçalves, Reginaldo Bezerra dos Santos, Jordi Miralda-Escudé, J. D. Hernández-Fernández, R. A. Dupke, Alberto Molino, R. Magalhães, L. Riguccini, A. Campillay, Ribamar R. R. Reis, Leandro Kerber, Fabricio Ferrari, G. B. Lima Neto, Pedro H. Bernardinelli, Stavros Akras, V. Branco, Devin D. Whitten, Luis Raul Weber Abramo, P. M. Novais, Antonio D. Montero-Dorta, S. Torres-Flores, Eduardo Telles, J. M. Carvano, C. E. Barbosa, R. de la Reza, Paulo A. A. Lopes, Alessandro Ederoclite
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 489:3403-3411
In this study we define a new sample of distant powerful radio galaxies in order to study their host-galaxy properties and provide targets for future observations of HI absorption with new radio telescopes and to understand the fuelling and feedback
Autor:
C. B. Oliveira, O. L. Dors, N. R. Telles, Angela Krabbe, Mónica V. Cardaci, Guillermo F. Hägele, J. A. Hernandez-Jimenez, Igor Zinchenko
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Chemical abundance determinations in Low-Ionization Nuclear Line Regions (LINERs) are especially complex and uncertain because the nature of the ionizing source of this kind of object is unknown. In this work, we study the oxygen abundance in relatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a001f7044cf9e279a0b7e4f26e00560e
http://arxiv.org/abs/2105.02072
http://arxiv.org/abs/2105.02072
Autor:
Guillermo F. Hägele, Angela Krabbe, I. C. Freitas, Mónica V. Cardaci, Nadia L. Zakamska, D. Ruschel-Dutra, Anna Feltre, Mark Kojo Armah, Thaisa Storchi-Bergmann, Rogemar A. Riffel, O. L. Dors, Enrique Pérez-Montero
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
We present maps for the electron temperature in the inner kpc of three luminous Seyfert galaxies: Mrk 79, Mrk 348, and Mrk 607 obtained from Gemini Multi-Object Spectrograph-integral field unit observations at spatial resolutions of ∼110–280 pc.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47677b4b708fe9caf12422dd22a85af6
http://arxiv.org/abs/2012.02013
http://arxiv.org/abs/2012.02013
Autor:
Max Faúndez-Abans, Angela Krabbe, Mónica V. Cardaci, Mark Kojo Armah, Enrique Pérez-Montero, E. B. Amôres, Guillermo F. Hägele, O. L. Dors, P. Freitas-Lemes
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Digital.CSIC. Repositorio Institucional del CSIC
instname
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Digital.CSIC. Repositorio Institucional del CSIC
instname
We compare the oxygen abundance (O/H) of the narrow-line regions (NLRs) of Seyfert 2 AGNs obtained through strong-line methods and from direct measurements of the electron temperature (Te-method). The aim of this study is to explore the effects of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb7b0a762d11d8da33f794cd0132ccd9
https://academic.oup.com/mnras/article/492/1/468/5679898
https://academic.oup.com/mnras/article/492/1/468/5679898
Autor:
Angela Krabbe, Guillermo F. Hägele, Mónica V. Cardaci, O. L. Dors, Enrique Pérez-Montero, Marcella Contini, Rogemar A. Riffel
Publikováno v:
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Consejo Superior de Investigaciones Científicas (CSIC)
Digital.CSIC. Repositorio Institucional del CSIC
instname
We build detailed composite models of photoionization and shock ionization based on the suma code to reproduce emission lines emitted from the Narrow Line Regions (NLR) of Seyfert 2 nuclei. The aim of this work is to investigate diagram active galact
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28c63c3d1f338bdbb0008d000786753d
Autor:
Guillermo F. Hägele, O. L. Dors, Angela Krabbe, Enrique Pérez-Montero, Mónica V. Cardaci, Mark Kojo Armah, S. P. Carvalho, A. F. Monteiro, P. Freitas-Lemes
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
instname
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We present a semi-empirical calibration between the metallicity (Z) of Seyfert 2 active galactic nuclei and the N2 = log([N HP.6584/11 cy) emission-line intensity ratio. This calibration was derived through the [0 m]..5007/[0 u[),3727 versus N2 diagr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4406402b07344e9572bfb5abc340ca4b
Autor:
Angela Krabbe, Roberto Maiolino, O. L. Dors, Mónica V. Cardaci, Guillermo F. Hägele, Mark Kojo Armah, Enrique Pérez-Montero
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
We investigate the discrepancy between oxygen abundance estimations for narrow-line regions of active galactic nuclei (AGNs) type Seyfert 2 derived using direct estimations of the electron temperature (T-e-method) and those derived using photoionizat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3c41f9e9dc897663f6d87058b557239c
http://hdl.handle.net/10261/221601
http://hdl.handle.net/10261/221601