Active Galactic Nuclei at the Crossroads of Astrophysics

Over the last five decades, AGN studies have produced a number of spectacular examples of synergies and multifaceted approaches in astrophysics. The field of AGN research now spans the entire spectral range and covers more than twelve orders of magnitude in the spatial and temporal domains. The next generation of astrophysical facilities will open up new possibilities for AGN studies, especially in the areas of high-resolution and high-fidelity imaging and spectroscopy of nuclear regions in the X-ray, optical, and radio bands. These studies will address in detail a number of critical issues in AGN research such as processes in the immediate vicinity of supermassive black holes, physical conditions of broad-line and narrow-line regions, formation and evolution of accretion disks and relativistic outflows, and the connection between nuclear activity and galaxy evolution.Comment: 16 pages, 5 figures; review contribution; "Exploring the Cosmic Frontier: Astrophysical Instruments for the 21st Century", ESO Astrophysical Symposia Serie

Reversal of infall in SgrB2(M) revealed by Herschel/HIFI observations of HCN lines at THz frequencies

International audienc

Herschel observations of extra-ordinary sources (HEXOS): Detecting spiral arm clouds by CH absorption lines

International audienc

Herschel observations of extra-ordinary sources (HEXOS): Detecting spiral arm clouds by CH absorption lines

International audienc

Oxidação lipídica do óleo de vísceras de aves para redução de seu conteúdo de energia metabolizável para frangos de corte na fase de crescimento Lipid oxidation decreases metabolizable energy value of dietary poultry fat for growing broilers

Com a finalidade de determinar os teores de energia metabolizável aparente (EMA) e de energia metabolizável aparente corrigida para o nitrogênio (EMAn) do óleo de vísceras de aves fresco e oxidado, foi conduzido um ensaio metabólico utilizando-se 48 machos AgRoss com 31 dias de idade. As aves foram alojadas em gaiolas metabólicas e o método utilizado foi o de coleta total de excretas. Foi fornecida uma dieta-referência com ou sem substituição de 10% pelo óleo de vísceras de aves fresco ou oxidado, sendo que cada dieta foi oferecida a quatro repetições de quatro aves. O período de coleta foi de quatro dias após três dias de adaptação às dietas e às gaiolas. O óleo de vísceras de aves foi adquirido de um produtor local e armazenado sob congelamento a -18&ordm;C (óleo fresco). O óleo oxidado foi obtido por aquecimento em banho-maria com temperatura entre 80 e 90&ordm;C. Durante o período de aquecimento, a qualidade deste óleo foi controlada por avaliações periódicas da absorbância específica, que indica o acúmulo de compostos de ranço. Os valores de absorbância específica, medidos a 232 e 270 nm, foram, respectivamente, de 4,64 e 0,47 para o óleo fresco e de 18,54 e 3,76 para o óleo oxidado. Os resultados obtidos, expressos na matéria original, para EMA e EMAn foram de 9.240 e 9.150 kcal/kg para o óleo de vísceras fresco e 7.700 e 7.595 kcal/kg para o óleo oxidado, comprovando estatisticamente grande redução no conteúdo de energia metabolizável do óleo decorrente do processo oxidativo.<br>In order to determine the apparent metabolizable energy (AME) and N-corrected apparent metabolizable energy (AMEn) of fresh and oxidized poultry fat a metabolism assay with 48 AgRoss male broilers from 31 to 34 days of age was conducted. The birds were fed a basal diet or this diet replaced by 10% of fresh or oxidized fat and the total excreta collection method was applied. The birds were housed in metabolic cages and each diet was supplied for four replicates of four birds. Fresh poultry fat was supplied by a local rendering and then stored frozen (-18&ordm;C). The oxidized poultry fat was obtained by heating (80 - 90&ordm;C) and specific absorbances were measured frequently to control fat quality. Specific absorbances at 232 and 270 nm were, respectively, 4.64 and 0.47 for fresh fat and 18.54 and 3.76 for oxidized fat, which suggest higher levels of conjugated dienes in the oxidized poultry fat. The results of AME and AMEn were 9,240 and 9,150 kcal/kg (as fed-basis) for the fresh poultry fat and 7,770 and 7,595 kcal/kg (as fed-basis) for the oxidized poultry fat. AME and AMEn values were statistically different, indicating a decrease in the energy from the fresh poultry fat to the oxidized fat due to oxidation

RESISTÊNCIA DE Colletotrichum fragariae E C. acutatum AO BENOMYL NA CULTURA DO MORANGO NO ESTADO DE SÃO PAULO

O fungicida benomyl, utilizado intensivamente na cultura do morango a partir do final da década de 60, tem sido ineficiente para o controle da flor preta, causada por Colletotrichum acutatum, devido ao aparecimento de formas resistentes ao fungicida, já detectadas desde 1984. Para C. fragariae, no entanto, não há registro de ocorrência de resistência no Estado de São Paulo, embora venha se observando há alguns anos que o produto não tem apresentado resultados satisfatórios para o controle da podridão do rizoma ("chocolate"). Para verificar a ocorrência de resistência em C. fragariae foram testados 22 isolados, coletados em diversas regiões produtoras de morango do Estado de São Paulo, e 22 isolados de C. acutatum, para comparação. Todos os isolados de C. acutatum foram resistentes, mesmo na concentração de 1000 ppm. Dos 22 isolados de C. fragariae, 10 comportaram-se como resistentes, crescendo em todas as concentrações testadas. Os demais só se desenvolveram até 1 ppm, sendo considerados sensíveis. As porcentagens de inibição do crescimento dos isolados de C. fragariae resistentes variaram de 50,0 a 88,8 (1 ppm), 54,5 a 89,8 (10 ppm), 63,6 a 78,7 (50 ppm), 67,3 a 80,3 (100 ppm), 74,4 a 82,0 (500 ppm) e 76,4 a 86,0 (1000 ppm). Inoculando-se isolados resistentes e sensíveis de C. fragariae em plantas da cultivar IAC-Campinas, observou-se que todos foram igualmente patogênicos.<br>The intensive use of benomyl in strawberry fields since the late 60s. resulted in an ineffective control of the flower blight, caused by Colletotrichum acutatum due to the development of resistance to the fungicide by the patogen, detected in 1984. Until recently, the resistance was not demonstrated in C. fragariae although an increasing failure of benomyl to provide satisfactory control of the crown rot ("chocolate" rot) has been observed, indicating the possible occurrence of resistance. To verify this evidence, 22 isolates of C. fragariae, collected at different localities in São Paulo State, were evaluated and compared with 22 isolates of C. acutatum. All the C. acutatum isolates were benomyl resistant, even at 1000 ppm. Among the 22 C. fragariae isolates, 10 were resitant. The percentages of mycelial growth inhibition of C. fragariae ranged from 50.0 to 88.8 (1 ppm), 54.5 to 89.8 (10 ppm), 63.6 to 78.7 (50 ppm), 67.3 to 80.3 (100 ppm), 74.4 to 82.0 (500 ppm) and 76.4 to 86.0 (1000 ppm). Resistant and sensitive isolates of C. fragariae were inoculated on strawberry plants of IAC-Campinas cultivar, causing similar symptoms

ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7

We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy to date, SPT-S J031132−5823.4 (hereafter SPT0311−58), at $z=6.900\pm 0.002$. SPT0311−58 was discovered via its 1.4 mm thermal dust continuum emission in the South Pole Telescope (SPT)-SZ survey. The spectroscopic redshift was determined through an Atacama Large Millimeter/submillimeter Array 3 mm frequency scan that detected CO(6–5), CO(7–6), and $[{\rm{C}}\,{\rm{I}}]$(2–1), and subsequently was confirmed by detections of CO(3–2) with the Australia Telescope Compact Array and $[{\rm{C}}\,{\rm{II}}]$ with APEX. We constrain the properties of the ISM in SPT0311−58 with a radiative transfer analysis of the dust continuum photometry and the CO and $[{\rm{C}}\,{\rm{I}}]$ line emission. This allows us to determine the gas content without ad hoc assumptions about gas mass scaling factors. SPT0311−58 is extremely massive, with an intrinsic gas mass of ${M}_{\mathrm{gas}}=3.3\pm 1.9\times {10}^{11}\,{M}_{\odot }$. Its large mass and intense star formation is very rare for a source well into the epoch of reionization