Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Veronica Menacho"'
Autor:
Alexandra Le Reste, Matthew Hayes, John M. Cannon, Edmund Christian Herenz, Jens Melinder, Veronica Menacho, Göran Östlin, Johannes Puschnig, T. Emil Rivera-Thorsen, Daniel Kunth, Nick Velikonja
Publikováno v:
The Astrophysical Journal. 934:69
The Lyα emission line is one of the main observables of galaxies at high redshift, but its output depends strongly on the neutral gas distribution and kinematics around the star-forming regions where UV photons are produced. We present observations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8eacc86817210238ff8e8973f4207878
https://doi.org/10.3847/1538-4357/ac77ed
https://doi.org/10.3847/1538-4357/ac77ed
Autor:
Veronica Menacho, Jens Melinder, Arjan Bik, G. Östlin, Thøger E. Rivera-Thorsen, L. Della Bruna, Nils Bergvall, Matthew Hayes, Angela Adamo
We use high quality VLT/MUSE data to study the kinematics and the ionized gas properties of Haro 11, a well known starburst merger system and the closest confirmed Lyman continuum leaking galaxy. We present results from integrated line maps, and from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fe73734141f6d034341a6b1faa1b074f
Autor:
G. Östlin, L. Della Bruna, Nils Bergvall, Angela Adamo, A. Bik, Veronica Menacho, Matthew Hayes, Jens Melinder, Edmund Christian Herenz
We have used the capability of the MUSE instrument to explore the impact of stellar feedback at large scales in Haro 11, a galaxy under extreme starburst condition and one of the first galaxies where Lyman continuum (LyC) has been detected. Using Ha,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c3e4ad46e8797ffeb4733a71a7746581
http://arxiv.org/abs/1903.11662
http://arxiv.org/abs/1903.11662
Autor:
Linda J. Smith, John M. Cannon, Jens Melinder, Daniel Kunth, Veronica Menacho, Axel Runnholm, Matteo Messa, Göran Östlin, Mattia Sirressi, T. Emil Rivera-Thorsen, M. S. Oey, Matthew Hayes, Arjan Bik, Genoveva Micheva, Peter Laursen, Angela Adamo, Max Gronke, J. Miguel Mas-Hesse
Publikováno v:
The Astrophysical Journal. 912:155
Understanding the escape of ionizing (Lyman continuum) photons from galaxies is vital for determining how galaxies contributed to reionization in the early universe. While directly detecting Lyman continuum from high redshift galaxies is impossible d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2d56059294a0927ed969f9a9731074f
https://doi.org/10.3847/1538-4357/abf1e8
https://doi.org/10.3847/1538-4357/abf1e8
Autor:
Matthew Hayes, Veronica Menacho, A. Bik, Göran Östlin, Angela Adamo, Jens Melinder, Edmund Christian Herenz
Publikováno v:
Astronomy & Astrophysics. 619:A131
Stellar feedback strongly affects the interstellar medium (ISM) of galaxies. Stellar feedback in the first galaxies likely plays a major role in enabling the escape of LyC photons, which contribute to the re-ionization of the Universe. Nearby starbur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be09ea4fd6864941203f4462929ff929
https://doi.org/10.1051/0004-6361/201833916
https://doi.org/10.1051/0004-6361/201833916
Autor:
Jens Melinder, Philippe Amram, Göran Östlin, Veronica Menacho, Matthew Hayes, Angela Adamo, Arjan Bik
Publikováno v:
NASA Astrophysics Data System
The stellar content of young massive star clusters emit large amounts of Lyman continuum photons and inject momentum into the inter stellar medium (ISM) by the strong stellar winds of the most massive stars in the cluster. When the most massive stars
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e9404c4c2befc40bafa7ce0c43264e64
http://arxiv.org/abs/1510.01944
http://arxiv.org/abs/1510.01944
Autor:
Veronica Menacho, Miguel Verdugo
Publikováno v:
Proceedings of the International Astronomical Union. 10:330-330
The origin of the morphology-density relation is still an open question in galaxy evolution. It is most likely driven by the combination of the efficient star formation in the highest peaks of the mass distribution at high-z and the transformation by
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fe20b7503d21126835635dbc6e79c32c
https://doi.org/10.1017/s1743921314010242
https://doi.org/10.1017/s1743921314010242