295 research outputs found

    Spin of protoplanets generated by pebble accretion: Influences of protoplanet-induced gas flow

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    We investigate the spin state of a protoplanet during the pebble accretion influenced by the gas flow in the gravitational potential of the protoplanet and how it depends on the planetary mass, the headwind speed, the distance from the host star, and the pebble size. We perform nonisothermal three-dimensional hydrodynamical simulations in a local frame to obtain the gas flow around the planet. We then numerically integrate three-dimensional orbits of pebbles under the obtained gas flow. Finally, assuming uniform spatial distribution of incoming pebbles, we calculate net spin by summing up specific angular momentum that individual pebbles transfer to the protoplanet at impacts. We find that a protoplanet with the envelope acquires prograde net spin rotation regardless of the planetary mass, the pebble size, and the headwind speed of the gas. This is because accreting pebbles are dragged by the envelope that commonly has prograde rotation. As the planetary mass or orbital radius increases, the envelope is thicker and the prograde rotation is faster, resulting in faster net prograde spin. When the dimensionless thermal mass of the planet, m=RBondi/Hm = R_{\mathrm{Bondi}} / H, where RBondiR_{\mathrm{Bondi}} and HH are the Bondi radius and the disk gas scale height, is larger than a certain critical mass (m0.3m \gtrsim 0.3 at 0.1au0.1 \, \mathrm{au} or m0.1m \gtrsim 0.1 at 1au1 \, \mathrm{au}), the spin rotation exceeds the breakup one. The predicted spin frequency reaches the breakup one at the planetary mass miso,rot0.1(a/1au)1/2m_{\mathrm{iso,rot}} \sim 0.1 \, (a / 1 \, \mathrm{au})^{-1/2} (where aa is the orbital radius), suggesting that the protoplanet cannot grow beyond miso,rotm_{\mathrm{iso,rot}}. It is consistent with the Earth's current mass and could help the formation of the Moon by a giant impact on fast-spinning proto-Earth.Comment: 14 pages, 10 figures, Accepted for publication in Astronomy and Astrophysics (A&A

    Description of a new species of the black fly subgenus Simulium (Ectemnaspis) from the Andes of Ecuador (Diptera: Simuliidae)

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    Simulium (Ectemnaspis) pautense sp. n. was described based on female, male, pupal and larval specimens collected in small streams of Andean region in Ecuador. This new species is close to S. (E.) gabaldoni Ramirez Perez from Venezuela by having the 6-filamented pupal gills, but differs in the female from the latter species by lacking denticles in the cibarium and by the coloration of the legs.Facultad de Ciencias Naturales y Muse

    The distribution and species diversity of black flies (Diptera: Simuliidae) in selected areas in Ranau, Sabah

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    Blackfly play an important role in the freshwater ecosystem as a biological indicator, as the blackfly prefers clean water area to breed. Certain blackfly species are categorized as vector as it can transmit disease known as Onchocerciasis (river blindness).This study is an entomology research which focuses on the species diversity of blackfly (Diptera: Simuliidae) in Ranau District of Sabah. Eight sampling stations located the highlands and lowlands were chosen. Larvae and pupae were manually collected directly from the substrate in the streams and river. A total of 12 data sets were collected over a period of six months, which started from August 2015 to January 2016. The data collection was done once every forth night. A preliminary result from this study has so far recorded fourteen species of blackfly. Among the fourteen species recorded, Simulium (Gomphostilbia) alienigenum was the first specimen recorded in Malaysia especially in Sabah. All the fourteen species of black flies recorded in this study belongs to three subgenus which are; Simulium, Nevermania and Gomphostilbia. The highest individual being recorded comes from the subgenus of Simulium. The diversity indices result shows a ranged from 1.13 to 1.58, and this indicates low diversity in the eight sampling stations

    The relationship between water quality and black fly (Diptera: Simuliidae) abundance in Tambunan District, Sabah

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    Black flies (Diptera : Simuliidae) have been extensively studied almost worldwide (Hamada & Grillet, 2001). This is because blackflies are among the best-known aquatic insects and globally distributed (Adler et al., 2004). Black flies in Malaysia are less known and research about this aquatic insect is still scarce especially in Borneo region. Most of the earlier studies on black flies in Sabah were related to taxonomy (Takaoka, 2001). However, studies on ecology and the role of black flies as bio-indicator has so far not been well reported yet. The aim of this study is to determine the relationship of water quality against the abundance of black flies pupa (Simuliidae). Regression test shows that relationship between dissolve oxygen (r2=0.57, p=0.02), total dissolve substance (TDS) (r2=0.18,p=0.04) and conductivity (r2=0.14, p=0.04) appeared significant to the abundance of black flies pupae. All the study sites (6 rivers) were classified into Class 1 based on Water Quality Index Classification (DOE, 2006)
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