ABSTRACT
Introduction: The order Euryalida is represented by fragile ophiuroids with long and slender arms that can be ramified. Species within the family Gorgonocephalidae are characterized by the presence of tiny hooklets on the dorsal aspect of their arms. There are very few published studies referring to species of the family Gorgonocephalidae inhabiting Mexican waters. Objective: To review the taxonomic status of the species belonging to this taxonomic family, identifying their diagnostic taxonomic characteristics to create an illustrated guide of species kept at the CNE, UNAM. Methods: Specialized bibliography of the Gorgonocephalidae family was gathered. Subsequently, all the specimens from the CNE were photographed using Scanning Electron and Multifocal Microscopy photography, to show the structures of taxonomic relevance. Results: A total of 193 specimens corresponding to eight genera and nine species were reviewed. The genus Astrocaneum presented the highest species richness. Conclusions: For the species identified in this study and for the sake of accurate identification, morphological characters such as the shape of hooklets and arm plates were highlighted.
Introducción: El orden Euryalida está formado por ofiuros frágiles con brazos delgados, largos y a veces ramificados. Las especies de la familia Gorgonocephalidae se caracterizan por la presencia de diminutos ganchos en el lado dorsal de sus brazos. Los estudios que refieren especies de la familia Gorgonocephalidae que habitan en aguas mexicanas son escasos. Objetivo: Realizar la revisión taxonómica de dicha familia, reconociendo los caracteres taxonómicos diagnósticos para generar una guía ilustrada de cada una de las especies que se encuentran en la CNE del ICML, UNAM. Métodos: Se recopiló toda la bibliografía especializada de la familia, posteriormente con ayuda de fotografías de MEB y multifocal se fotografiaron los especímenes de la CNE para destacar las estructuras de importancia taxonómica. Resultados: se revisaron un total de 193 ejemplares correspondientes a ocho géneros, nueve especies, siendo el género Astrocaneum el de mayor riqueza específica. Conclusiones: Para las especies identificadas en este estudio, para dar una identificación más precisa, se destacaron los caracteres morfológicos forma de los ganchos y forma de las placas de los brazos.
Subject(s)
Animals , Starfish/classification , Echinodermata/classification , MexicoABSTRACT
Objective:To investigate the extent of statistics anxiety and explore its influencing factors among university students majoring in medicine.Methods:The statistics anxiety rating scale (STARS) was first translated into Chinese and modified until the reliability and validity were acceptable. Through online questionnaire, the Chinese version of STARS was used to measure the level of statistics anxiety for students enrolling in the course of Medical Statistics during autumn term 2018 to spring term 2019 in the medical college of a university. The collected data were managed and analyzed by SPSS 25.0.Results:A total of 562 students took part in the survey, and 500 questionnaires were eligible and included in the final analysis. The measurement of Chinese version of STARS showed quite good reliability and validity, with item score of the whole scale being (2.31 ± 0.65) points. The proportions of students with mild, moderate and severe statistics anxiety were 41%, 56% and 3% respectively. Female students had higher extent of anxiety than male students, and undergraduates had higher extent of anxiety than postgraduates. The extent of anxiety of students with different majors from high to low were nursing > (dentistry, basic medicine and pharmacology) > (clinic medicine and public health) respectively. When controlling other factors, the influence of gender, student level and major on statistics anxiety was still statistically significant.Conclusion:Statistics anxiety is prevalent in medical college students. Professional teachers should pay more attention to students' psychological status, conduct targeted counseling to alleviate students' anxiety and help them to improve self-efficacy in statistics learning.
ABSTRACT
Abstract Despite the important effort of knowing the Ophiuroidea diversity in the Mexican Pacific, some mistakes in the taxonomic nomenclature have pervaded through time. In order to clarify the latter, a checklist based on literature review of brittle stars from the Mexican Pacific is provided. We reviewed a total of 105 references that in total summarized 125 species of brittle stars from the Mexican Pacific (112) and the Gulf of California (97), belonging to two orders, 16 families and 50 genera. These records are higher than those reported on previous studies carried out in the area. México is the country with the highest number of brittle stars reported in the Tropical Eastern Pacific; this may be due to its exceptional oceanographic conditions, location and coastline extension. However, a total of 27 species reported in the literature were considered doubtful due to their general distributions and were not included in the checklist. Of the reported species, 35 have their type locality in the Mexican Pacific, corroborating the importance of the country in the Tropical Eastern Pacific in terms of Echinodermata diversity. Rev. Biol. Trop. 63 (Suppl. 2): 37-47. Epub 2015 June 01.
Resumen A pesar del importante esfuerzo en el conocimiento de la diversidad de ofiuroideos del Pacífico mexicano, algunos errores en la nomenclatura taxonómica han perseverado a través del tiempo. Con el objetivo de clarificar lo anterior, se provee una lista de especies de ofiuroideos del Pacífico Mexicano, basada en la revisión de literatura. Se revisó un total de 105 referencias que en total suman 125 especies pertenecientes a dos órdenes, 16 familias y 50 géneros de ofiuros del Pacífico Mexicano (112) y el Golfo de California (97). Estos reportes son mayores que otros estudios llevados a cabo en el área. México es el país con el mayor número de ofiuros reportados en el Pacífico Oriental Tropical; esto puede deberse a su excepcional condición oceanográfica, ubicación y extensión de línea de costa. Un total de 27 de las especies reportadas en la literatura fueron consideradas dudosas de acuerdo distribución geográfica por lo que no fueron incluidas en la lista. 35 especies poseen su localidad tipo en el Pacífico Mexicano, corroborando la importancia de México en el Pacífico Oriental Tropical en términos de diversidad de equinodermos.
Subject(s)
Animals , Starfish/classification , Echinodermata/classification , MexicoABSTRACT
Abstract The post-metamorphic stage is essential in the life history of marine invertebrates. During this period, animals are more vulnerable and suffer high mortality, which influences the distribution and abundance of adult populations. It is also during this period that major morphological changes happen in the individuals, complicating their taxonomic identification. The juvenile ophiuroids dominate the meiofauna in certain times of the year and at some places. However, they are ignored by most ecological studies due to identification difficulties. Here we describe the ontogeny of nine deep-sea species from the Southeast and South regions of Brazil, with the first record of morphological modifications for eight of them. Most organisms were collected 60 to 800 m deep, between December 1997, January, 1998 and March, 1998, during the REVIZEE-Score South / Benthos program. We also included additional material from the Zoology Museum of Unicamp (ZUEC). For descriptions and identifications of the different stages, the specimens were dried and photographed. The juveniles were identified by "backwards" process through the growth series of adults to smaller individuals, a backwards method that was successful in previous studies. Some individuals were mounted on aluminum stubs for scanning electron microscopy. The species were: Ophiacantha pentacrinus (Ophiacanthidae), Ophiomastus satelitae, Ophiomusium acuferum, Ophiomusium eburneum, Ophiomisidium tommasii, Ophiura ljungmani, Ophiura clemens (Ophiuridae), Amphiura complanata (Amphiuridae) and Ophiothrix rathbuni (Ophiotrichidae). Many species could be identified since their most juvenile stage. Some structures remain almost unaltered during the whole life. Rev. Biol. Trop. 63 (Suppl. 2): 361-381. Epub 2015 June 01.
Resumen La etapa post-metamórfica es esencial en la historia de vida de los invertebrados marinos. Durante este período, los animales son más vulnerables y sufren una elevada mortalidad, que influye en la distribución y abundancia de las poblaciones de los adultos. También es durante este período cuando grandes cambios morfológicos ocurren en los individuos, lo que complica su identificación taxonómica. Los ofiuroideos juveniles son el componente principal para la mayor parte de la composición de la meiofauna en ciertas épocas del año y en algunos lugares. Sin embargo, son ignorados por la mayoría de los estudios ecológicos debido a las dificultades de identificación. De esta manera, la descripción de las fases juveniles presenta mayor importancia, sobre todo en estudios relacionados con la dinámica poblacional y de composición de fauna. Este trabajo tiene como objetivo describir la ontogenia de nueve especies de aguas profundas de las regiones Sudeste y Sur de Brasil, siendo el primer registro en la literatura sobre cambios morfológicos -a partir del crecimiento- para ocho de ellos. La mayoría de los organismos se tomaron en el intervalo de 60 a 800 m de profundidad, entre diciembre de 1997, enero de 1998 y marzo de 1998, durante el programa REVIZEE Sur-Score / Bentos. También se incluyen en este estudio material adicional del Museo de Zoología de la Unicamp (ZUEC). Para las identificaciones y descripciones de las diferentes etapas, las muestras se secaron y fueron fotografiadas. Los juveniles fueron identificados por "al revés" el proceso de crecimiento a través de la serie desde adultos hasta los individuos de menores tallas, una metodología exitosa en estudios anteriores. Las especies seleccionadas para la descripción de la serie de crecimiento fueron escogidas de acuerdo a su abundancia relativa en diferentes etapas de desarrollo. Algunos individuos fueron montados en tacos de aluminio para la microscopía electrónica de barrido. Las especies se estudiadas fueron: Ophiacantha pentacrinus (Ophiacanthidae), Ophiomastus satelitae, Ophiomusium acuferum, Ophiomusium eburneum, Ophiomisidium tommasii, Ophiura ljungmani, Ophiura clemens (Ophiuridae), Amphiura complanata (Amphiuridae) y Ophiothrix rathbuni (Ophiotrichidae). El análisis del desarrollo post-metamórfico de los individuos reveló que muchas especies podrían ser identificadas desde sus etapas más juveniles, sobre todo a partir de caracteres morfológicos externos. Este estudio nos permite sostener que algunas estructuras permanecen casi inalteradas durante toda la vida del organismo, mientras que otras están sujetas a transformaciones. De este modo, se contribuye al conocimiento más amplio de algunas especies de ofiuroideos, con relación a la caracterización de sus diferentes etapas de desarrollo.
Subject(s)
Animals , Starfish/classification , Benthic Fauna/classification , Classification , Hydrobiology/classification , Invertebrates/classification , Atlantic OceanABSTRACT
El formalismo de la relatividad general es usado para calcular el radio de la órbita marginalmente estable (ROME), las frecuencias kepleriana, de Lense-Thirring, de precesion y oscilación de los movimientos radiales y verticales, de una partícula de prueba neutra que orbita el plano ecuatorial de una estrella de neutrones magnetizada. El espacio tiempo alrededor de la estrella se modela por medio de la solución seis paramétrica derivada por Pachón et al. (2012). Se concluye que la presencia del campo magnético de la fuente tiene efectos apreciables en las cantidades físicas mencionadas arriba y, por tanto, su inclusión es necesaria si se desea describir con más exactitud los procesos físicos que ocurren en la vecindad de este tipo de estrellas tales como la dinámica de discos de acreción. Los resultados presentados aquí también sugieren que la presencia de campos magnéticos intensos pueden introducir correcciones apreciables en, por ejemplo, las predicciones de la masa de estrellas de neutrones hechas con base en el modelo de precesión relativista.
A full-relativistic approach is used to compute the radius of the innermost stable circular orbit (ISCO), the Keplerian, frame-dragging, precession and oscillation frequencies of the radial and vertical motions of neutral test particles orbiting the equatorial plane of a magnetized neutron star. The space-time around the star is modelled by the six parametric solution derived by Pachón et al. (2012) It is shown that the inclusion of an intense magnetic field, such as the one of a neutron star, have non-negligible effects on the above physical quantities, and therefore, its inclusion is necessary in order to obtain a more accurate and realistic description of physical processes, such as the dynamics of accretion disks, occurring in the neighbourhood of this kind of objects. The results discussed here also suggest that the consideration of strong magnetic fields may introduce non-negligible corrections in, e.g., the relativistic precession model and therefore on the predictions made on the mass of neutron stars.
O formalismo da relatividade geral é usado para calcular o raio da órbita marginalmente estável (ROME), as frequencias keplerianas de Lense Thirring, precessao e oscilaçao de movimentos radiais e verticais, de uma partícula de prova neutra em órbita equatorial de uma estrela de neutrón magnetizada. O espaço-tempo ao redor da estrela é modelado por meio da soluçao seis paramétrica derivada por Pachón et al. (2012). Conclui-se que a presença do campo magnético da fonte tem efeitos apreciáveis nas quantidades físicas mencionadas acima e, portanto, a sua inclusão é necessária se se deseja descrever com mais exatidão os processos físicos que ocorrem na vizinhança deste tipo de estrelas tais como a dinâmica dos discos de acreção. Os resultados apresentados também sugerem que a precessão de campos magnéticos intensos podem introduzir correcções apreciáveis em, por exemplo, as predições da massa da estrela de neutróns feitas com base nos modelos de precessão relativista.
ABSTRACT
There is limited biological information about the starfish Oreaster reticulatus and the nine-armed starfish Luidia senegalensis in Venezuelan waters. These species are currently considered threatened in many localities of the Caribbean, Brazil and Colombia. Therefore, the aim of this study was to describe their population density, size distribution and population structure in Cubagua Island. During 2008, 52 stations located around the island were evaluated using band transects of 50m2. Each organism was counted and measured (maximum radius), and its size was compared to the maturity length reported in the literature. The results for O. reticulatus include: 167.3ind./ha; 33% juveniles and 67% adults; average size of 10.7±5cm (range: 2.2-21cm); a wide distribution around the island, with higher densities in the Eastern and Southwest areas. The 50% of the specimens were found in seagrass beds, 25% in sand, 16% in areas covered by decomposed seaweeds, 9% in oyster beds and 1% coralline patches. The densities of O. reticulatus were higher than those reported in the Caribbean, Panama and Puerto Rico, but lower than Venezuelan National Parks: Mochima and Morrocoy; as well as in the Virgin Islands and Belize. For L. senegalensis we found an average density of 40ind./ha; 95% exceeded the reported size at maturity, with mean length of 12cm±3.5cm (range: 3.5-22.3cm); they were found only in 15% of the stations of which 92.5% were sandy bottoms and the other 7.5% oyster beds. The degree of aggregation of L. senegalensis was greater than O. reticulatus, with an estimated k of 0.06. However, it was not possible to compare the densities of L. senegalensis with any other study. For both species is recommended to carry out reproductive studies and to monitor their population densities to infer temporal variations.
Las estrellas de mar: Oreaster reticulatus y Luidia senegalensis, han sido objeto de escasos estudios en aguas venezolanas. Actualmente son consideradas especies amenazadas en diversas zonas del Caribe, Brasil y Colombia. Por esto, se planteó como objetivo generar información sobre su densidad poblacional, distribución y estructura de talla en los alrededores de la isla de Cubagua. Para ello, durante el año 2008, se realizaron cuatro transectas bandas de 50m2 cada una, en 52 estaciones ubicadas alrededor de la isla. Entre los resultados obtenidos para O. reticulatus destacan: 167.3ind/ha, un 33% inmaduros y 67% adultos con un promedio de tallas de 10.7±5cm (rango: 2.2-21cm); una amplia distribución en los alrededores de la isla, con mayores densidades en la zona este y suroeste. Luidia senegalensis mostró una densidad promedio de 40ind/ha, 95% superaba la talla de madurez reportada, con talla promedio de 12cm±3.5cm (rango: 3.5-22.3cm). Se recomienda realizar estudios de reproducción, así como monitoreos de sus densidades poblacionales que permitan inferir sus variaciones temporales.