Zobrazeno 1 - 10
of 86
pro vyhledávání: '"Bernhard Aringer"'
Autor:
Paola Marigo, Peter Woitke, Emanuele Tognelli, Léo Girardi, Bernhard Aringer, Alessandro Bressan
Publikováno v:
The Astrophysical Journal, Vol 960, Iss 1, p 18 (2023)
In this study we compute the equation of state and Rosseland mean opacity from temperatures of T ≃ 30,000 K down to T ≃ 400 K, pushing the capabilities of the Æ SOPUS code into the regime where solid grains can form. The GGchem code is used to s
Externí odkaz:
https://doaj.org/article/c648cb3297dd40a7a532c22615992159
Autor:
Danny Gasman, Ioannis Argyriou, G. C. Sloan, Bernhard Aringer, Javier Álvarez-Márquez, Ori Fox, Alistair Glasse, Adrian Glauser, Olivia C. Jones, Kay Justtanont, Patrick J. Kavanagh, Pamela Klaassen, Alvaro Labiano, Kirsten Larson, David R. Law, Michael Mueller, Omnarayani Nayak, Alberto Noriega-Crespo, Polychronis Patapis, Pierre Royer, Bart Vandenbussche
Publikováno v:
Astronomy & Astrophysics, 673
Context. The Medium Resolution Spectrometer (MRS) is one of the four observing modes of JWST/MIRI. Using JWST in-flight data of unresolved (point) sources, we can derive the MRS absolute spectral response function (ASRF) starting from raw data. Spect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aada6fa1678dc00dec63718a3379f1d9
https://hdl.handle.net/20.500.11850/615000
https://hdl.handle.net/20.500.11850/615000
Autor:
Alessandro Bressan, Martin Groenewegen, Bernhard Aringer, Martha L. Boyer, Jacco Th. van Loon, Ambra Nanni, S. Rubele, S. R. Goldman
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2019, 487, pp.502-521. ⟨10.1093/mnras/stz1255⟩
Monthly Notices of the Royal Astronomical Society, 2019, 487, pp.502-521. ⟨10.1093/mnras/stz1255⟩
The properties of carbon stars in the Magellanic Clouds (MCs) and their total dust production rates are predicted by fitting their spectral energy distributions (SED) over pre-computed grids of spectra reprocessed by dust. The grids are calculated as
Publikováno v:
Astronomy and Astrophysics
The winds observed around AGB stars are generally attributed to radiation pressure on dust formed in the dynamical atmospheres of these long-period variables. The composition of wind-driving grains is affected by a feedback between their optical prop
Autor:
Giada Pastorelli, Sara Bladh, Jason S. Kalirai, Pierre Bergeron, Sihao Cheng, Léo Girardi, Piero Dal Tio, Bernhard Aringer, Alessandro Bressan, Pier-Emmanuel Tremblay, Enrico Ramirez-Ruiz, Paola Marigo, Jason L. Curtis, Michele Trabucchi, Yang Chen, Jeffrey D. Cummings
Publikováno v:
Nature Astronomy
The initial-final mass relation (IFMR) links the birth mass of a star to the mass of the compact remnant left at its death. While the relevance of the IFMR across astrophysics is universally acknowledged, not all of its fine details have yet been res
Autor:
Franz Kerschbaum, Bernhard Aringer, M. Mecina, M. Brunner, Martin Groenewegen, Walter Nowotny, Hans-Peter Gail
Context. Stars on the asymptotic giant branch lose considerable amounts of matter through their dust-driven stellar winds. A number of such sources have been imaged by Herschel/PACS, revealing a diverse sample of different morphological types. Among
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69d18b0d5d76bb297f859fffc4efbf77
Publikováno v:
Proceedings of the International Astronomical Union. 14:391-393
We have improved the treatment of dust opacity from the small-particle limit approximation to size-dependent which leads to models with smaller grains, lower dust-to-gas ratios, but about the same mass-loss rates and outflow velocities. The K-magnitu
The atmospheres and winds of C-type AGB stars are modeled with the 1D spherically symmetric radiation-hydrodynamical code DARWIN. To explore the metallicity-dependence of mass loss we calculate model grids at three different chemical abundances. Sinc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dd548af008b6c03c4d28098c322431e8
http://arxiv.org/abs/1902.05352
http://arxiv.org/abs/1902.05352
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2019, 487, pp.2133-2147. ⟨10.1093/mnras/stz1429⟩
Monthly Notices of the Royal Astronomical Society, 2019, 487, pp.2133-2147. ⟨10.1093/mnras/stz1429⟩
We have computed a grid of hydrostatic spherical COMARCS models for C stars covering metallicities from [Z/H]=0 to -2 and values of the carbon excess [C-O] from 6.41 to 9.15, plus some temperature sequences, where the amount of oxygen and nitrogen is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eca4941a6c5b0dff1f95fd001507996c
http://hdl.handle.net/11577/3309172
http://hdl.handle.net/11577/3309172
Autor:
Bernhard Aringer, Giada Pastorelli, Léo Girardi, Martha L. Boyer, Peter R. Wood, Julianne J. Dalcanton, Yang Chen, S. Bladh, Philip Rosenfield, Susanne Höfner, Josefina Montalbán, Maria-Rosa L. Cioni, Martin Groenewegen, Alessandro Bressan, S. Rubele, Paola Marigo, Ambra Nanni, Michele Trabucchi, Kjell Eriksson, Thomas Lebzelter
Publikováno v:
Monthly Notices of the Royal Astronomical Society
The thermally-pulsing asymptotic giant branch (TP-AGB) experienced by low- and intermediate-mass stars is one of the most uncertain phases of stellar evolution and the models need to be calibrated with the aid of observations. To this purpose, we cou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c3af13a2841a67faf18f9007ab1d19e3
http://hdl.handle.net/20.500.11767/108185
http://hdl.handle.net/20.500.11767/108185