Sobre a relação entre rotação, atividade crosmosférica e abundância de lítio em estrelas subgigantes

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Cranial osteology and systematic implications in Crotophaginae (Aves, Cuculidae)

Recognizing the scarcity of anatomical and phylogenetic studies on Crotophaginae, the authors set Out to add to the anatomical knowledge of the group based on a detailed description of cranial osteology. Another objective was to verify whether this source of data could be used to infer relationships by performing the first cladistic analysis of the four species of Crotophaginae. The shortest-length cladogram (consistency index = 1.0) indicated that cranial osteology is an important source of characters for cladistic analysis of cuckoos. The findings corroborated the monophyly of Crotophaginae, showing that Guira guira is (lie most divergent and plesiomorphic taxon and that Crotophaga ani and Crotophaga sulcirostris are more closely related to each other than to Crotophaga major.

Um estudo da abundância de lítio, rotação, atividade cromosférica e magnetismo das estrelas análogas e gêmeas solares

The study physical process that control the stellar evolution is strength influenced by several stellar parameters, like as rotational velocity, convective envelope mass deepening, and magnetic field intensity. In this study we analyzed the interconnection of some stellar parameters, as Lithium abundance A(Li), chromospheric activity and magnetic field intensity as well as the variation of these parameters as a function of age, rotational velocity, and the convective envelope mass deepening for a selected sample of solar analogs and twins stars. In particular, we analyzed the convective envelope mass deepening and the dispersion of lithium abundance for these stars. We also studied the evolution of rotation in subgiants stars, because its belong to the following evolutionary stage of solar analogs, and twins stars. For this analyze, we compute evolutionary models with the TGEC code to derive the evolutionary stage, as well as the convective envelope mass deepening, and derive more precisely the stellar mass, and age for this 118 stars. Our Investigation shows a considerable dispersion of lithium abundance for the solar analogs stars. We also realize that this dispersion is not by the convective zone deep, in this way we observed which the scattering of A(Li) can not be explained by classical theories of mixing in the convective zone. In conclusion we have that are necessary extra-mixing process to explain this decrease of Lithium abundance in solar analogs and twins stars. We analyzed the subgiant stars because this are the subsequent evolutionary stage after the solar analogs and twins stars. For this analysis, we compute the rotational period for 30 subgiants stars observed by Co- RoT satellite. For this task we apply two different methods: Lomb-Scargle algorithm, and the Plavchan Periodogram. We apply the TGEC code we compute models with internal distribution of angular momentum to confront the predict results with the models, and the observational results. With this analyze, we showed which solid body rotation models are incompatible with the physical interpretation of observational results. As a result of our study we still concluded that the magnetic field, convective envelope mass deepening, and internal redistribution of angular momentum are essential to explain the evolution of low-mass stars, and its observational characteristics. Based on population synthesis simulation, we concluded that the solar neighborhood presents a considerable quantity of solar twins when compared with the discovered set nowadays. Altogether we foresee the existence around 400 solar analogs in the solar neighborhood (distance of 100 pc). We also study the angular momentum of solar analogs and twins, in this study we concluded that added angular momentum from a Jupiter type planet, putted in the Jupiter position, is not enough to explain the angular momentum predicted by Kraft law (Kraft 1970)

Evolução da atividade cromosférica, abundância de lítio e rotação das estrelas análogas e gêmeas solares

The study of solar-type stars also includes the familiar solar analogs and twins. These objects have been one of the major research subjects in astrophysics nowadays. A direct comparison of solar activity with chromospheric activity indices for a set of stars very similar to the Sun (twins and analogs) provides an excellent opportunity to study the evolution of stellar activity on timescales of the order of the lifetime on the main sequence. This work deals with the relationship between the abundance of lithium, chromospheric activity, X-ray emission and rotation period in terms of stellar ages. We explore the influence of stellar evolution in the global properties of the stars and the aspects linked to its coronal, chromospheric and magnetic activity. Our main objective is to probe the law of decay of each of these parameters based on a sample of stars classified as well-connected as analogs stars and solar twins.

Sobre a relação entre rotação, atividade crosmosférica e abundância de lítio em estrelas subgigantes

The connection between rotation, CaII emission flux and lithium abundance is analyzed for a sample of subgiant stars, with evolutionary status was determined from the Toulouse-Geneve code and HlPPARCOS trigonometric parallax measurements. We noted that the distribution of rotation and CaII emission flux, as a function of effective temperature, shows a discontinuity located around the same spectral type, F8IV. Stars located blueward of this spectral type, exhibit a large spread of values of rotation and CaII flux, whereas stars redward of F8lV show essentially low ratation anel low CaII flux. The strength of these declines nevertheless, depends on stellar mass. The distribution of lithium abundances also shows a discontinuity, however with behavior a little more complex for subgiants with mass lower than about 1.2 Solar Masses, this decrease is observed later than that in rotation and CaII flux, whereas for masses higher than 1.2 Solar Masses the decrease in lithium abundance is located around the spectral type F8IV. The discrepancy between the location of the discontinuities of rotation and CaII flux and log n(Li) for stars with masses lower than 102 Solar Masses, seems to reflect the sensitivity of these phenomena to the mass of the convective envelope. The drop in rotation, which results mostly from a magnetic braking, requires an increase in the mass of the convective envelope less than that required for the decrease in lithium abundance The location of the discontinuity in log n( Li) in the same region of the discontinuity ties in rotation and CaII flux, for stars with masses higher than 1.2 Solar Masses, may also be explained by the behavior of the deepening of the convective envelope. In contrast to the relationship between rotation and CaII flux the relationship between lithium abundance and rotation shows no dear tendency toward linear behavior. Similarly, the same tendency is observed in the relationship between lithium abundance and CaII flux in spite of these facts, subgiants with high lithium content also have high rotation and high CaII emission flux. We also observed that stars with high lithium content present, in its majority, an undeveloped convective envelope, whereas stars with low lithium content have a developed convective envelope. In the case of the rotation, stars with undeveloped convective envelope, show rotational velocities as much high as low, whereas stars with developed convective envelope only present low rotation

Taxonomia e biogeografia da espécie politípica Herpsilochmus rufimarginatus (TEMMINCK, 1822) (Aves: THAMNOPHILIDAE)

The genus Herpsilochmus is composed mainly of cryptic species, among them is Herpsilochmus rufimarginatus, which is currently represented by four subspecies: H. r. rufimarginatus, H. r. frater, H. r. scapularis and H. r. exiguus. Differences in plumage and vocalization suggest that there are more than one species involved in this complex. Thus this and other subspecific taxa need urgent revision, the disjunct distribution of this species also allows us to infer the relationship between birds that occur in this biome and / or different centers of endemism. This study aims to make a taxonomic revision of the taxa included in the complex time Herpsilochmus rufimarginatus based on morphological, morphometric, vocals and geographical distribution of this bird. Besides creating distribution models current potential and make the reconstruction of the distribution bygone using ecological niche modeling, and testing the niche conservatism and divergence between different subspecies. Consultations for examination of the skins of specimens of the museums: Museum of Zoology, University of São Paulo (MZUSP), National Museum of Rio de Janeiro (MN) and Emilio Goeldi Museum of Pará (MPEG), and the skins deposited at the collection of Ornithological Federal University of Rio Grande do Norte (COUFRN). We studied the following measures length of specimens: exposed culmen, culmen and total culmen nostril, tarsus, wing and tail flattened. The voice analysis was performed with vocalizations banks and / or digital banks people where 17 voice parameters were measured. This information and more available in the literature were used to assemble a bunch of data under the limit distribution of taxa and generate ecological niche models. This analyzes carried out in the program Maxent, having as model selection criterion the AUC, and the models were greater than 0.80 are considered good models. Environmental data for the realization of the modeling were downloaded on the website of Worldclim. The morphometric information, vocals and geographic distribution point for the separation of these taxa to be considering various uni and multivariate analyzes. The potential distribution models performed well (AUC> 0.80), and its distribution associated with environmental characteristics of the Amazon forest and Atlantic forest (forests of south and southeast, northeast and forest). The reconstruction of the distribution indicates a possible contact between the southern part of the Atlantic forest in the northern part of the Amazon. The analysis of niche overlap showed a low overlap between taxa and comparisons between the null model and the generated overlay link probably occurring niche conservatism. The data suggest that the taxa that occur in the Amazon and Atlantic forest represent three distinct species

Efeito da microbiota cecal e do Lactobacillus salivarius inoculados in ovo em aves desafiadas com Salmonella enterica sorovar Enteritidis

Ovos embrionados provenientes de matrizes pesadas foram inoculados na câmara de ar com microbiota cecal total, microbiota cecal diluída e cultura de Lactobacillus salivarius, no 18º dia de incubação. Dois dias após o nascimento, as aves foram desafiadas com Salmonella enterica sorovar Enteritidis (SE) e, cinco dias após o desafio, avaliou-se a presença da bactéria no fígado e ceco. O efeito de exclusão competitiva, após o desafio com SE, somente foi observado pela ausência da bactéria no fígado das aves tratadas in ovo com L. salivarius. A inoculação in ovo de microbiota cecal indefinida ou diluída não reduziu a colonização de SE no fígado e no ceco das aves, incluindo, neste último, também o tratamento com L. salivarius. Nenhum dos tratamentos in ovo determinou índice de eclodibilidade superior a 65%.

Avaliação in vitro da atividade inibitória de Lactobacillus spp., isolados do inglúvio e cecos de aves sobre Salmonella

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Comparação entre método bioquímico e reação em cadeia de polimerase para identificação de Lactobacillus spp., isolados de aves

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Rastreabilidade de farinha de vísceras de aves por isótopos estáveis em penas de frangos de corte

O objetivo deste trabalho foi detectar a presença de farinha de vísceras de aves (FV) na alimentação de frangos de corte, por meio da análise de penas por isótopos estáveis de carbono (13C/12C) e nitrogênio (15N/14N) e espectrofotometria de massas. Setecentos e vinte pintos machos Cobb foram submetidos aos seguintes tratamentos: ração vegetal (RV) à base de milho e farelo de soja, de 1 a 42 dias de idade; ração com 8% de farinha de vísceras de frango (FV), de 1 a 42 dias de idade; ração vegetal de 1 a 21 dias e ração com FV de 22 a 42 dias; ração vegetal de 1 a 35 dias e ração com FV de 36 a 42 dias; ração com FV de 1 a 21 dias, e ração vegetal de 22 a 42 dias; ração com FV de 1 a 35 dias, e ração vegetal de 36 a 42 dias. Foram colhidas amostras de penas de quatro aves por tratamento aos 7, 14, 21, 28, 35 e 42 dias de idade, que foram submetidas à análise isotópica de carbono (13C/12C) e nitrogênio (15N/14N) por espectrometria de massas. A aplicação da técnica dos isótopos estáveis de C e N a penas de frango de corte, após a utilização de farinha de vísceras na alimentação de frangos de corte, pelo período de até 21 dias, permite detectar a inclusão da FV na dieta.

Composição e abundância dos caranguejos (Decapoda, Brachyura) nas regiões de Ubatuba e Caraguatatuba, litoral norte paulista, Brasil

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Anurofauna em área de cerrado aberto no município de Borebi, estado de São Paulo, Sudeste do Brasil: uso do habitat, abundância e variação sazonal

O bioma Cerrado encontra-se descaracterizado e menos de três por cento de suas áreas originais está legalmente protegida. A anurofauna desse bioma não é muito rica quando comparado a outros biomas, porém há um grande número de espécies endêmicas. Aqui apresentamos uma lista de espécies de anuros registrados em uma lagoa em área de cerrado aberto do município de Borebi, região Centro-Oeste do estado de São Paulo, sudeste do Brasil. Durante 24 meses de estudo (2008 e 2009) caracterizamos a distribuição das espécies na lagoa estudada e descrevemos a variação sazonal das espécies. Foram registradas 27 espécies pertencentes a seis famílias: Bufonidae (duas espécies), Cycloramphidae (uma espécie), Hylidae (13 espécies), Leiuperidae (quatro espécies), Leptodactylidae (cinco espécies) e Microhylidae (duas espécies). A riqueza de espécies e abundância estiveram relacionadas com a precipitação. Dendropsophus minutus foi a espécie mais abundante e com registro de vocalização durante o ano inteiro. Rhinella ornata e Odontophrynus americanus foram restritas ao período seco e frio (abril a agosto). As outras espécies tiveram seu período de maior atividade nos meses chuvosos e quentes (setembro a março). A ocupação da lagoa variou com o tipo de vegetação e conforme a variação do seu volume de água, principalmente nos período de estiagem. A alta riqueza e abundância de anuros da lagoa pode ser resultado da ausência de peixes predadores, dos diversos tipos de microambientes do local e da ausência de outros corpos d'água próximos.

Composição e abundância da ictiofauna de duas lagunas costeiras da América do Sul Austral: lagoa do Peixe (31ºS; 51ºW), Brasil e laguna Mar Chiquita (37ºS; 57ºW), Argentina

This article describes and compares the shallow water fish-fauna from two coastal lagoons (Peixe Lagoon, in Brazil, and Mar Chiquita Lagoon, in Argentina). Peixe Lagoon was sampled between 2000 and 2001 using a 9 m beach seine net (12 mm bar mesh in the wings and 5 mm in the centre 3 m section) totalizing 125 samples, which yielded 33,848 individuals and 32 species. Mar Chiquita Lagoon was sampled from 1995 to 1998 using a 21) m beach seine net (12 mm bar mesh) totalizing 232 samples resulting in 31,097 individuals of 28 species. A total of 47 species were observed in both lagoons and 13 were shared. The "marine-estuarine-related" species were similar and dominate the fish assemblages in both lagoons. The remaining species were similar to the species collected along the southern Brazil, Uruguay and Argentina estuaries. The number of species observed in Peixe Lagoon (S = 32) was higher than in Mar Chiquita Lagoon (S = 28) and is probably associated with a strong latitudinal gradient of species richness increasing from north to south. Considering that the Peixe Lagoon and Mar Chiquita Lagoon are isolated by the large estuaries of Patos Lagoon and Prata River, the composition of the species with low abundance and occasional occurrence were different for each local studied. These results expand the knowledge for the fauna of both sites and help conservation and management from both lagoons.

Distribuição e abundância de espécies arbóreas em cerradões no Pantanal, Estado do Mato Grosso do Sul, Brasil

Os cerradões no Pantanal ocorrem em áreas não inundáveis da planície e são importantes para a economia regional. Das áreas de cerradão são retiradas madeiras para construção de cercas, currais e galpões. Apesar da grande importância dos recursos vegetais do cerradão, existem poucas informações para embasar sua conservação e uso sustentável. Este trabalho teve como objetivos estudar a abundância, a distribuição das espécies arbóreas e correlações com a fertilidade do solo em áreas de cerradão (savana florestada) do Pantanal Sul Mato-grossense. Foram estudadas seis áreas de cerradão na sub-região da Nhecolândia, por meio de 30 pontos quadrantes, totalizando 120 árvores amostradas, com circunferência a altura do peito (CAP) > 15 cm, em cada área. As comparações florísticas, de abundância das espécies e de fertilidade do solo, foram efetuadas por análises de componentes principais (PCA). As áreas mostraram-se heterogêneas, apresentando diferentes níveis de fertilidade do solo, estrutura e composição da vegetação. Dois cerradões foram agrupados em termos de fertilidade do solo e de estrutura da vegetação, apresentando muitas árvores de Qualea grandiflora Mart., espécie que ocorreu associada a solos com maiores teores de fósforo. Outros dois cerradões apresentaram composição florística mais semelhante que os demais, apesar de ocorrerem em solos com diferentes níveis de fertilidade, indicando perturbação antrópica.

Aves como potenciais dispersoras de sementes de Ocotea pulchella Mart. (Lauraceae) numa área de vegetação de cerrado do sudeste brasileiro

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)