Zobrazeno 1 - 10
of 53
pro vyhledávání: '"Matthias Maercker"'
Autor:
M. Andriantsaralaza, Raghvendra Sahai, Taissa Danilovich, Sofia Ramstedt, Hans Olofsson, Martin Groenewegen, Maryam Saberi, Susanne Höfner, Franz Kerschbaum, E. De Beck, Albert A. Zijlstra, Matthias Maercker, Theo Khouri, G. Quintana-Lacaci, Wouter Vlemmings, Michael Lindqvist
Publikováno v:
Astronomy and Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
25 pags., 15 figs., 4 tabs.
Aims. We aim to constrain the sizes of, and investigate deviations from spherical symmetry in, the CO circumstellar envelopes (CSEs) of 16 S-type stars, along with an additional 7 and 4 CSEs of C-type and M-type AGB s
Aims. We aim to constrain the sizes of, and investigate deviations from spherical symmetry in, the CO circumstellar envelopes (CSEs) of 16 S-type stars, along with an additional 7 and 4 CSEs of C-type and M-type AGB s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::445b75147d15391af3190794b4d381a0
https://lirias.kuleuven.be/handle/123456789/682658
https://lirias.kuleuven.be/handle/123456789/682658
Autor:
S. Ramstedt, L.-Å. Nyman, John H. Black, Matthias Maercker, Daniel Tafoya, Theo Khouri, Wouter Vlemmings, Hans Olofsson, E. M. L. Humphreys, Michael Lindqvist
We report the detection of two lines at millimetre wavelengths towards the immediate surroundings of the post-giant and most likely post-common-envelope star HD101584 using high-angular-resolution ALMA observations. The circumstellar environment of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b4025a52e8e4b8ab6d96bdd80a6ff134
Autor:
Matthias Maercker, Franz Kerschbaum, Martin Groenewegen, Hans Olofsson, Susanne Höfner, Daniel Tafoya, L. Doan, Rodolfo Montez, Theo Khouri, Taissa Danilovich, Wouter Vlemmings, E. De Beck, Raghvendra Sahai, Albert A. Zijlstra, Sofia Ramstedt, G. Quintana-Lacaci, Maryam Saberi, Michael Lindqvist, Joel H. Kastner
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
28 pags., 10 figs., 7 tabs.
Context. This is the first publication from the DEATHSTAR project. The overall goal of the project is to reduce the uncertainties of the observational estimates of mass-loss rates from evolved stars on the Asymptotic
Context. This is the first publication from the DEATHSTAR project. The overall goal of the project is to reduce the uncertainties of the observational estimates of mass-loss rates from evolved stars on the Asymptotic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fcd50482661c701840561fecf9cc9d5f
http://hdl.handle.net/10261/224210
http://hdl.handle.net/10261/224210
Autor:
Pierre Kervella, Claudia Paladini, Matthias Maercker, A. de Koter, Wouter Vlemmings, Christian Ginski, Eric Lagadec, L. B. F. M. Waters, E. De Beck, Leen Decin, Theo Khouri
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A200. ⟨10.1051/0004-6361/201834618⟩
Astronomy & Astrophysics, 635:A200. EDP Sciences
Astronomy & Astrophysics, 635, A200
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A200. ⟨10.1051/0004-6361/201834618⟩
Astronomy & Astrophysics, 635:A200. EDP Sciences
Astronomy & Astrophysics, 635, A200
Stars with initial masses between $\sim0.8$ and 8~$M_\odot$ present copious mass loss during the asymptotic giant branch (AGB) at the end of their lives. The accepted mass-loss mechanism requires radiation pressure acting on dust grains that form in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::84245c6b3fcee5f048dc53a2c9fed8a2
https://lirias.kuleuven.be/handle/123456789/654046
https://lirias.kuleuven.be/handle/123456789/654046
Autor:
Christian Ginski, Hans Olofsson, Wouter Vlemmings, Elvire De Beck, Theo Khouri, Matthias Maercker, Sofia Ramstedt
Publikováno v:
Proceedings of the International Astronomical Union. 14:31-35
The mass-loss mechanism of asymptotic giant branch stars has long been thought to rely on two processes: stellar pulsations and dust formation. The details of the mass-loss mechanism have remained elusive, however, because of the overall complexity o
Autor:
L. Doan, Michael Lindqvist, Wouter Vlemmings, Franz Kerschbaum, Claudia Paladini, S. Höfner, S. Mohamed, S. Ramstedt, E. De Beck, Matthias Maercker, Markus Wittkowski
The AGB star $\pi^{1}$ Gruis has a known companion (at a separation of ~400 AU) which cannot explain the strong deviations from the spherical symmetry of the CSE. Recently, hydrodynamic simulations of mass transfer in closer binary systems have succe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e210173045332bf5a59320f4b9ce691
http://arxiv.org/abs/1911.10756
http://arxiv.org/abs/1911.10756
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 463:L74-L78
We report the serendipitous detection with ALMA of the vibrationally-excited pure-rotational CO transition $v=1, J=3-2$ towards five asymptotic giant branch (AGB) stars, $o$ Cet, R Aqr, R Scl, W Aql, and $\pi^1$ Gru. The observed lines are formed in
Autor:
Wouter Vlemmings, Michael Lindqvist, Jacques Kluska, Matthias Maercker, Daniel Tafoya, H. Van Winckel, E. M. L. Humphreys, Hans Olofsson, Markus Wittkowski, Sofia Ramstedt, W. J. de Wit, Theo Khouri
Publikováno v:
Astronomy & Astrophysics. 642:A152
Context: The observed orbital characteristics of post-asymptotic giant branch (post-AGB) and post-red giant branch (post-RGB) binaries are not understood. We suspect that the missing ingredients to explain them probably lie in the continuous interact
Autor:
Hans Olofsson, Theo Khouri, Alain Baudry, Elizabeth Humphreys, E. De Beck, Wouter Vlemmings, Guillermo Garcia-Segura, Matthias Maercker, Sofia Ramstedt, Eva Villaver
Publikováno v:
Astronomy and Astrophysics (0004-6361) vol.613(2018)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, pp.id.L4. ⟨10.1051/0004-6361/201832929⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, pp.id.L4. ⟨10.1051/0004-6361/201832929⟩
High resolution observations of the extended atmospheres of asymptotic giant branch (AGB) stars can now directly confront the theories that describe stellar mass loss. Using Atacama Large Millimeter/submillimeter Array (ALMA) high angular resolution
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7ece1a8304d3a26fe7f7dd16f5dd8642
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-357271
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-357271
Autor:
M. Mecina, Ernst A. Dorfi, M. Brunner, Hans Olofsson, Franz Kerschbaum, Matthias Maercker, Gioia Rau
Aims. The carbon-rich asymptotic giant branch (AGB) star TX Piscium (TX Psc) has been observed multiple times during multiple epochs and at different wavelengths and resolutions, showing a complex molecular CO line profile and a ring-like structure i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f48f38d133d60c2b322bd67b7c23072