Zobrazeno 1 - 10
of 4 708
pro vyhledávání: '"Anna A T"'
Autor:
Kirk, James, Ahrer, Eva-Maria, Claringbold, Alastair B., Zamyatina, Maria, Fisher, Chloe, McCormack, Mason, Panwar, Vatsal, Powell, Diana, Taylor, Jake, Thorngren, Daniel P., Christie, Duncan A., Esparza-Borges, Emma, Tsai, Shang-Min, Alderson, Lili, Booth, Richard A., Fairman, Charlotte, López-Morales, Mercedes, Mayne, N. J., Meech, Annabella, Molliere, Paul, Owen, James E., Penzlin, Anna B. T., Sergeev, Denis E., Valentine, Daniel, Wakeford, Hannah R., Wheatley, Peter J.
We present a transmission spectrum of the misaligned hot Jupiter WASP-15b from 2.8--5.2 microns observed with JWST's NIRSpec/G395H grating. Our high signal to noise data, which has negligible red noise, reveals significant absorption by H$_2$O ($4.2\
Externí odkaz:
http://arxiv.org/abs/2410.08116
Autor:
Penzlin, Anna B. T., Booth, Richard A., Nelson, Richard P., Schäfer, Christoph M., Kley, Wilhelm
Many of the most intriguing features, including spirals and cavities, in the current disc observations are found in binary systems like GG Tau, HD 142527 or HD 100453. Such features are evidence of the dynamic interaction between binary stars and the
Externí odkaz:
http://arxiv.org/abs/2407.07243
Autor:
Kirk, James, Ahrer, Eva-Maria, Penzlin, Anna B. T., Owen, James E., Booth, Richard A., Alderson, Lili, Christie, Duncan A., Claringbold, Alastair B., Esparza-Borges, Emma, Fisher, Chloe E., López-Morales, Mercedes, Mayne, N. J., McCormack, Mason, Meech, Annabella, Panwar, Vatsal, Powell, Diana, Taylor, Jake, Sergeev, Denis E., Valentine, Daniel, Wakeford, Hannah R., Wheatley, Peter J., Zamyatina, Maria
A primary objective of exoplanet atmosphere characterisation is to learn about planet formation and evolution, however, this is challenged by degeneracies. To determine whether differences in atmospheric composition can be reliably traced to differen
Externí odkaz:
http://arxiv.org/abs/2407.03198
Autor:
Penzlin, Anna B. T., Booth, Richard A., Kirk, James, Owen, James E., Ahrer, Eva-Maria, Christie, Duncan A., Claringbold, Alastair B., Esparza-Borges, Emma, López-Morales, M., Mayne, N. J., McCormack, Mason, Meech, Annabella, Panwar, Vatsal, Powell, Diana, Sergeev, Denis E., Taylor, Jake, Wheatley, Peter J., Zamyatina, Maria
Hot Jupiters present a unique opportunity for measuring how planet formation history shapes present-day atmospheric composition. However, due to the myriad pathways influencing composition, a well-constructed sample of planets is needed to determine
Externí odkaz:
http://arxiv.org/abs/2407.03199
Autor:
Gurina, Ekaterina
Publikováno v:
The Journal of Education, Culture, and Society. 9(2):218-225
Externí odkaz:
https://www.ceeol.com/search/article-detail?id=693133
Autor:
Afkanpour, Zahra, Ataiee, Sareh, Ziampras, Alexandros, Penzlin, Anna B. T., Sfair, Rafael, Schäfer, Christoph, Kley, Wilhelm, Schlichting, Hilke
Publikováno v:
A&A 686, A277 (2024)
Resonant planetary migration in protoplanetary discs can lead to an interplay between the resonant interaction of planets and their disc torques called overstability. While theoretical predictions and N-body simulations hinted at its existence, there
Externí odkaz:
http://arxiv.org/abs/2404.05791
Publikováno v:
Il Foro Italiano, 2007 Jan 01. 130(1), 137/138-161/162.
Externí odkaz:
https://www.jstor.org/stable/23202560
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:
Adelbert, Stefan, Penzlin, Anna B. T., Schäfer, Christoph M., Kley, Wilhelm, Quarles, Billy, Sfair, Rafael
Publikováno v:
A&A 680, A29 (2023)
In previous hydrodynamical simulations, we found a mechanism for nearly circular binary stars, like Kepler-413, to trap two planets in a stable 1:1 resonance. Therefore, the stability of coorbital configurations becomes a relevant question for planet
Externí odkaz:
http://arxiv.org/abs/2310.07575
Autor:
Elizabeth Blackwell
Publikováno v:
Scientific and Medical Knowledge Production, 1796-1918 ISBN: 9781003009450
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4c15d79bc382145f253ed82f43e16eae
https://doi.org/10.4324/9781003009450-13
https://doi.org/10.4324/9781003009450-13