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Observações de Gaia e Kepler do Novo Catálogo 6811 a partir da lente de Uganda

Observações de Gaia e Kepler do Novo Catálogo 6811 a partir da lente de Uganda

Doris Atino Eggo

64,24 €
IVA incluido
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Editorial:
KS OmniScriptum Publishing
Año de edición:
2025
Materia
Tecnología aeroespacial y aeronáutica
ISBN:
9786206822653
64,24 €
IVA incluido
Disponible

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Sobre IBD

Foi efectuado um estudo fotométrico extensivo do aglomerado para determinar o avermelhamento, a distância, a idade e a metalicidade do aglomerado entre as estrelas de magnitude ≤ 18 (estrelas brilhantes). As estrelas de magnitude > 18 (estrelas fracas) foram deixadas de fora, criando assim uma lacuna na filiação do NGC 6811 (Curtis et al. 2019). Assim, o problema abordado foi que o número de estrelas binárias fracas conhecidas com componente δ scuti no aglomerado aberto NGC 6811 ainda é pequeno. Este estudo contribuiu para o número de estrelas δ scuti fracas conhecidas neste aglomerado usando o segundo lançamento de dados do Kepler e Gaia (DR2).

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Otros libros del autor

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  • Observations Gaia et Kepler du nouveau catalogue 6811 à partir de la lentille Ouganda
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    Une étude photométrique approfondie de l’amas pour déterminer le rougissement de l’amas, la distance, l’âge et la métallicité a été réalisée parmi les étoiles de magnitude ≤ 18 (étoiles brillantes). Les étoiles de magnitude > 18 (étoiles faibles) ont été laissées de côté, créant ainsi une lacune dans l’appartenance à NGC 6811 (Curtis et al. 2019). Ainsi, le problème abordé étai...
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  • Osservazioni Gaia e Kepler del nuovo catalogo 6811 dalla lente Uganda
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    Un ampio studio fotometrico dell’ammasso per determinare l’arrossamento dell’ammasso, la distanza, l’età e la metallicità è stato effettuato tra le stelle di magnitudine ≤ 18 (stelle luminose). Le stelle di magnitudine > 18 (stelle deboli) sono state escluse, creando così una lacuna nell’appartenenza a NGC 6811 (Curtis et al. 2019). Il problema affrontato era quindi che il nume...
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  • Obserwacje Gaia i Kepler nowego katalogu 6811 z obiektywu Uganda
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    Obszerne badanie fotometryczne gromady w celu określenia zaczerwienienia gromady, odległości, wieku i metaliczności zostało przeprowadzone wśród gwiazd o jasności ≤ 18 (jasne gwiazdy). Gwiazdy o magnitudo > 18 (słabe gwiazdy) zostały pominięte, tworząc lukę w członkostwie NGC 6811 (Curtis et al. 2019). W ten sposób rozwiązano problem polegający na tym, że liczba znanych słabych...
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