Zobrazeno 1 - 10
of 1 350
pro vyhledávání: '"Kratter"'
Autor:
Buccini Luca, Benedetti Francesca, Kratter Matilde, Mura Francesco, Proietti Anacleto, Atanasio Pierfrancesco, Cirigliano Angela, Rossi Marco, Rinaldi Teresa, Passeri Daniele
Publikováno v:
BIO Web of Conferences, Vol 129, p 27011 (2024)
Externí odkaz:
https://doaj.org/article/264b9039767547f98fc72fa6b8857dd7
Autor:
Mura Francesco, Benedetti Francesca, Kratter Matilde, Buccini Luca, Atanasio Pierfrancesco, Proietti Anacleto, Cirigliano Angela, Passeri Daniele, Rinaldi Teresa, Rossi Marco
Publikováno v:
BIO Web of Conferences, Vol 129, p 27007 (2024)
Externí odkaz:
https://doaj.org/article/007b19815f88408c9249aac4ee2cef66
The spin-orbit alignment of binary stars traces their formation and accretion history. Previous studies of spin-orbit alignment have been limited to small samples, slowly rotating solar-type stars, and/or wide visual binaries that not surprisingly ma
Externí odkaz:
http://arxiv.org/abs/2408.05329
Autor:
Zariski, Jackson, Kratter, Kaitlin, Logsdon, Sarah, Bender, Chad, Li, Dan, Schweiker, Heidi, Rajagopal, Jayadev, McBride, Bill, Hunting, Emily
The WIYN 3.5m Telescope at Kitt Peak National Observatory hosts a suite of optical and near infrared instruments, including an extreme precision, optical spectrograph, NEID, built for exoplanet radial velocity studies. In order to achieve sub ms prec
Externí odkaz:
http://arxiv.org/abs/2407.08046
Autor:
Krapp, Leonardo, Kratter, Kaitlin M., Youdin, Andrew N., Benítez-Llambay, Pablo, Masset, Frédéric, Armitage, Philip J.
The formation of circumplanetary disks is central to our understanding of giant planet formation, influencing their growth rate during the post-runaway phase and observability while embedded in protoplanetary disks. We use 3D global multifluid radiat
Externí odkaz:
http://arxiv.org/abs/2402.14638
Autor:
Duffell, Paul C., Dittmann, Alexander J., D'Orazio, Daniel J., Franchini, Alessia, Kratter, Kaitlin M., Penzlin, Anna B. T., Ragusa, Enrico, Siwek, Magdalena, Tiede, Christopher, Wang, Haiyang, Zrake, Jonathan, Dempsey, Adam M., Haiman, Zoltan, Lupi, Alessandro, Pirog, Michal, Ryan, Geoffrey
We have performed numerical calculations of a binary interacting with a gas disk, using eleven different numerical methods and a standard binary-disk setup. The goal of this study is to determine whether all codes agree on a numerically converged sol
Externí odkaz:
http://arxiv.org/abs/2402.13039
Autor:
Reynolds, Nickalas K., Tobin, John J., Sheehan, Patrick D., Sadavoy, Sarah I., Looney, Leslie W., Kratter, Kaitlin M., Li, Zhi-Yun, Segura-Cox, Dominique M., Kaib, Nathan A.
We present a statistical characterization of circumstellar disk orientations toward 12 protostellar multiple systems in the Perseus molecular cloud using the Atacama Large Millimeter/submillimeter Array at Band 6 (1.3 mm) with a resolution of 25 mas
Externí odkaz:
http://arxiv.org/abs/2312.13570
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 Explicit (I
Externí odkaz:
http://arxiv.org/abs/2310.04435
Autor:
Moe, Maxwell, Kratter, Kaitlin M.
Solar-type binaries with short orbital periods (P-close equivalent to 1-10. days; a less than or similar to 0.1. au) cannot form directly via fragmentation of molecular clouds or protostellar disks, yet their component masses are highly correlated, s
Externí odkaz:
http://hdl.handle.net/10150/627100
http://arizona.openrepository.com/arizona/handle/10150/627100
http://arizona.openrepository.com/arizona/handle/10150/627100
Autor:
Cox, Erin G., Harris, Robert J., Looney, Leslie W., Chiang, Hsin-Fang, Chandler, Claire, Kratter, Kaitlin, Li, Zhi-Yun, Perez, Laura, Tobin, John J.
We present a high angular resolution (similar to 0 ''.2), high-sensitivity (sigma similar to 0.2 mJy) survey of the 870 mu m continuum emission from the circumstellar material around 49 pre-main-sequence stars in the rho Ophiuchus molecular cloud. Be
Externí odkaz:
http://hdl.handle.net/10150/626413
http://arizona.openrepository.com/arizona/handle/10150/626413
http://arizona.openrepository.com/arizona/handle/10150/626413