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pro vyhledávání: '"Strampelli, Giovanni Maria"'
Autor:
Robberto, Massimo, Gennaro, Mario, Da Rio, Nicola, Strampelli, Giovanni Maria, Ubeda, Leonardo, Sabbi, Elena, Koeppe, Dana, Tan, Jonathan C., Soderblom, David R.
We performed a HST/WFC3-IR imaging survey of the young stellar cluster NGC 2024 in three filters probing the 1.4~$\mu$m H$_2$O absorption feature, characteristic of the population of low mass and sub-stellar mass objects down to a few Jupyter masses.
Externí odkaz:
http://arxiv.org/abs/2310.04888
Autor:
Smith, Nathan, Rest, Armin, Andrews, Jennifer E., Matheson, Tom, Bianco, Federica B., Prieto, Jose L., James, David J., Smith, R. Chris, Strampelli, Giovanni Maria, Zenteno, A.
In our ongoing study of eta Carinae's light echoes, there is a relatively bright echo that has been fading slowly, reflecting the 1845-1858 plateau of the eruption. A separate paper discusses its detailed evolution, but here we highlight one importan
Externí odkaz:
http://arxiv.org/abs/1808.00991
Light-echoes from the plateau in Eta Carinae's Great Eruption reveal a two-stage shock-powered event
Autor:
Smith, Nathan, Andrews, Jennifer E., Rest, Armin, Bianco, Federica B., Prieto, Jose L., Matheson, Tom, James, David J., Smith, R. Chris, Strampelli, Giovanni Maria, Zenteno, A.
We present multi-epoch photometry and spectroscopy of a light echo from eta Carinae's 19th century Great Eruption. This echo shows a steady decline over a decade, sampling the 1850s plateau of the eruption. Spectra show the bulk outflow speed increas
Externí odkaz:
http://arxiv.org/abs/1808.00992
Akademický článek
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Autor:
Robberto, Massimo, Gennaro, Mario, Ubeira Gabellini, Maria Giulia, Hillenbrand, Lynne A., Pacifici, Camilla, Ubeda, Leonardo, Andersen, Morten, Barman, Travis, Bellini, Andrea, Da Rio, Nicola, de Mink, Selma E., Lodato, Giuseppe, Manara, Carlo Felice, Platais, Imants, Pueyo, Laurent, Strampelli, Giovanni Maria, Tan, Jonathan C., Testi, L.
In order to obtain a complete census of the stellar and substellar population, down to a few M_(Jup) in the ~1 Myr old Orion Nebula Cluster, we used the infrared channel of the Wide Field Camera 3 of the Hubble Space Telescope with the F139M and F130
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________38::d1a60c92f97fe237e63984dc4021e499
https://resolver.caltech.edu/CaltechAUTHORS:20200622-104136068
https://resolver.caltech.edu/CaltechAUTHORS:20200622-104136068
Autor:
Robberto, Massimo, Gennaro, Mario, Gabellini, Maria Giulia Ubeira, Hillenbrand, Lynne A., Pacifici, Camilla, Ubeda, Leonardo, Andersen, Morten, Barman, Travis, Bellini, Andrea, Da Rio, Nicola, de Mink, Selma E., Lodato, Giuseppe, Manara, Carlo Felice, Platais, Imants, Pueyo, Laurent, Strampelli, Giovanni Maria, Tan, Jonathan C., Testi, L.
Publikováno v:
Astrophysical Journal; 6/10/2020, Vol. 896 Issue 1, p1-20, 20p