Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Juan Garrido-Deutelmoser"'
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 271, Iss 1, p 7 (2024)
We present MDIRK: a multifluid second-order diagonally implicit Runge–Kutta method to study momentum transfer between gas and an arbitrary number ( N ) of dust species. The method integrates the equations of hydrodynamics with an implicit–explici
Externí odkaz:
https://doaj.org/article/75bd200db62345afa6bc2dbc419f720f
Autor:
Juan Garrido-Deutelmoser, Cristobal Petrovich, Carolina Charalambous, Viviana V. Guzmán, Ke Zhang
Publikováno v:
The Astrophysical Journal Letters, Vol 945, Iss 2, p L37 (2023)
The Atacama Large Millimeter Array observations of the disk around HD 163296 have resolved a crescent-shape substructure at around 55 au, inside and off-center from a gap in the dust that extends from 38 to 62 au. In this work we propose that both th
Externí odkaz:
https://doaj.org/article/f567ba472d984b5baeeb78b5ddfde957
Autor:
Carolina Charalambous, Juan Garrido-Deutelmoser, Viviana Guzman, Cristobal Petrovich, Ke Zhang
ALMA observations of the disk around HD 163296 have resolved a crescent-shape substructure at around 55 au, inside and off-center from a gap in the dust that extends from 38 au to 62 au. In this work we propose that both the crescent and the dust rin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28162b7237ff3299ddbfa6b039c6f80b
http://arxiv.org/abs/2301.13260
http://arxiv.org/abs/2301.13260
Autor:
Juan Garrido-Deutelmoser, Cristobal Petrovich, Leonardo Krapp, Kaitlin M. Kratter, Ruobing Dong
The substructures observed in protoplanetary disks may be the signposts of embedded planets carving gaps or creating vortices. The inferred masses of these planets often fall in the Jovian regime despite their low abundance compared to lower-mass pla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8864602dc1b2d2b8d5cd354080ea5156
Autor:
Juan Garrido-Deutelmoser, Johan Olofsson, Nicolás Cuello, Jorge Cuadra, Matías Montesinos, C. A. Giuppone, Amelia Bayo, Mario Sucerquia
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy & Astrophysics
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy & Astrophysics
Trojans are defined as objects that share the orbit of a planet at the stable Lagrangian points $L_4$ and $L_5$. In the Solar System, these bodies show a broad size distribution ranging from micrometer($\mu$m) to centimeter(cm) particles (Trojan dust
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9db31943a201d5fc0c7acc45560d4fcb