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  • 1
    In: The Astronomical Journal, American Astronomical Society, Vol. 161, No. 4 ( 2021-04-01), p. 194-
    Abstract: We present the discovery and characterization of five hot and warm Jupiters—TOI-628 b (TIC 281408474; HD 288842), TOI-640 b (TIC 147977348), TOI-1333 b (TIC 395171208, BD+47 3521A), TOI-1478 b (TIC 409794137), and TOI-1601 b (TIC 139375960)—based on data from NASA’s Transiting Exoplanet Survey Satellite (TESS). The five planets were identified from the full-frame images and were confirmed through a series of photometric and spectroscopic follow-up observations by the TESS Follow-up Observing Program Working Group. The planets are all Jovian size ( R P = 1.01–1.77 R J ) and have masses that range from 0.85 to 6.33 M J . The host stars of these systems have F and G spectral types (5595 ≤ T eff ≤ 6460 K) and are all relatively bright (9.5 〈 V 〈 10.8, 8.2 〈 K 〈 9.3), making them well suited for future detailed characterization efforts. Three of the systems in our sample (TOI-640 b, TOI-1333 b, and TOI-1601 b) orbit subgiant host stars ( g 〈 4.1). TOI-640 b is one of only three known hot Jupiters to have a highly inflated radius ( R P 〉 1.7 R J , possibly a result of its host star’s evolution) and resides on an orbit with a period longer than 5 days. TOI-628 b is the most massive, hot Jupiter discovered to date by TESS with a measured mass of M J and a statistically significant, nonzero orbital eccentricity of e = . This planet would not have had enough time to circularize through tidal forces from our analysis, suggesting that it might be remnant eccentricity from its migration. The longest-period planet in this sample, TOI-1478 b ( P = 10.18 days), is a warm Jupiter in a circular orbit around a near-solar analog. NASA’s TESS mission is continuing to increase the sample of well-characterized hot and warm Jupiters, complementing its primary mission goals.
    Type of Medium: Online Resource
    ISSN: 0004-6256 , 1538-3881
    RVK:
    Language: Unknown
    Publisher: American Astronomical Society
    Publication Date: 2021
    detail.hit.zdb_id: 2207625-6
    detail.hit.zdb_id: 2003104-X
    SSG: 16,12
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  • 2
    Online Resource
    Online Resource
    Universidade Estadual de Maringa ; 2020
    In:  Revista Tecnológica Vol. 29, No. 2 ( 2020-04-17), p. 526-540
    In: Revista Tecnológica, Universidade Estadual de Maringa, Vol. 29, No. 2 ( 2020-04-17), p. 526-540
    Abstract: Os agregagos de resíduos da construção civil e demolição (RCD) possuem grande potencial de aplicação em obras de drenagem e pavimentação, quando atendidos os requisitos previstos pelas normas técnicas vigentes. Pesquisas apontam para a possível quebra de grãos mediante esforços de compactação no campo. Assim, esta pesquisa teve como objetivo avaliar a viabilidade de uso de RCD e mistura solo-RCD em camadas de pavimentos, bem como uma avaliação da potencial quebra dos agregados durante o processo de compactação e após análises de Índice de Suporte Califórnia (CBR) e compressão edométrica. Os limites de consistência indicaram o RCD como redutor de plasticidade. Através dos resultados obtidos constatou-se que o RCD e a mistura solo-RCD atendem aos requisitos de CBR e expansão para reuso como material de reforço do subleito, sub-base e até base de pavimentos para determinados teores de umidade. Na análise de quebra, identificou-se menor resistência do RCD em relação a mistura solo-RCD. Os índices de quebra determinados mostraram mudanças na distribuição granulométrica do RCD e da mistura solo-RCD como dependentes do teor de umidade do material. Os resultados indicaram que a quebra dos grãos ocorre com maior intensidade para os agregados do RCD em altas tensões, sugerindo o uso da mistura solo-RCD.
    Type of Medium: Online Resource
    ISSN: 2447-2476 , 1517-8048
    Language: Unknown
    Publisher: Universidade Estadual de Maringa
    Publication Date: 2020
    detail.hit.zdb_id: 2650256-2
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