Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Dalal El Youssoufi"'
Autor:
Dalal El Youssoufi, Maria-Rosa L Cioni, Nikolay Kacharov, Cameron P M Bell, Gal Matjević, Kenji Bekki, Richard de Grijs, Valentin D Ivanov, Jacco Th van Loon
We present a kinematic analysis of the Small Magellanic Cloud using 3700 spectra extracted from the European Southern Observatory archive. We used data from Gaia and near-infrared photometry to select stellar populations and discard Galactic foregrou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::03999f1739c8e53922be1f29a4ab9a58
Autor:
Cameron P. M. Bell, Dalal El Youssoufi, Smitha Subramanian, Thomas Schmidt, Jacco Th. van Loon, Valentin D. Ivanov, Maria-Rosa L. Cioni, Kenji Bekki, Ning-Chen Sun, S. Rubele, Jonathan Diaz, Richard de Grijs, Florian Niederhofer, Joana M. Oliveira, Gal Matijevic, Vincenzo Ripepi
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 502:2859-2878
We used data from the near-infrared VISTA survey of the Magellanic Cloud system (VMC) to measure proper motions (PMs) of stars within the Small Magellanic Cloud (SMC). The data analysed in this study comprise 26 VMC tiles, covering a total contiguous
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28684de597adb51d1270fb992a200ee3
https://doi.org/10.1093/mnras/stab206
https://doi.org/10.1093/mnras/stab206
Autor:
Thomas Schmidt, Maria-Rosa L. Cioni, Florian Niederhofer, Kenji Bekki, Cameron P. M. Bell, Richard de Grijs, Dalal El Youssoufi, Valentin D. Ivanov, Joana M. Oliveira, Vincenzo Ripepi, Jacco Th. van Loon
Publikováno v:
Astronomy and Astrophysics
The Large Magellanic Cloud (LMC) is the most luminous satellite galaxy of the Milky Way and owing to its companion, the Small Magellanic Cloud (SMC), represents an excellent laboratory to study the interaction of dwarf galaxies. The aim of this study
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f7086abb9b46959c3b53f143de7ae9d1
https://doi.org/10.1051/0004-6361/202142148
https://doi.org/10.1051/0004-6361/202142148
Autor:
Vincenzo Ripepi, Maria-Rosa L. Cioni, Dalal El Youssoufi, Martin Groenewegen, Jacco Th. van Loon, Thomas Schmidt, Florian Niederhofer, Richard de Grijs, Gal Matijevic, Valentin D. Ivanov, Smitha Subramanian, Joana M. Oliveira, Ning-Chen Sun, Cameron P. M. Bell
We study the morphology of the stellar periphery of the Magellanic Clouds in search of substructure using near-infrared imaging data from the VISTA Hemisphere Survey (VHS). Based on the selection of different stellar populations using the ($J-K_\math
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45521d84bc22ca6c4f376076b97e0817
http://arxiv.org/abs/2104.08054
http://arxiv.org/abs/2104.08054
Autor:
Adhya Mary, Kenji Bekki, Dalal El Youssoufi, Smitha Subramanian, Abinaya O. Omkumar, Jacco Th. van Loon, Dizna James, Maria-Rosa L. Cioni, Richard de Grijs, Florian Niederhofer, Sreeja S. Kartha
The eastern region of the Small Magellanic Cloud (SMC) is found to have a foreground stellar sub-structure, which is identified as a distance bimodality (12 kpc apart) in the previous studies using Red Clump (RC) stars. Interestingly, studies of Red
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d9f668c66f78750e70f8af7a0654760
Autor:
Maria-Rosa L. Cioni, Florian Niederhofer, Abinaya O. Omkumar, Smitha Subramanian, Dalal El Youssoufi, Jacco Th. van Loon, Richard de Grijs, Jonathan Diaz, Kenji Bekki
Recent observational studies identified a foreground stellar sub-structure traced by red clump (RC) stars (~ 12 kpc in front of the main body) in the eastern regions of the Small Magellanic Cloud (SMC) and suggested that it formed during the formatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::33ba33281cd9b1f415f8a953871df744
http://arxiv.org/abs/2010.02687
http://arxiv.org/abs/2010.02687
Autor:
Thomas Schmidt, Vincenzo Ripepi, Richard de Grijs, Anna B. A. Queiroz, Monika G. Petr-Gotzens, Cameron P. M. Bell, Jim Emerson, Dalal El Youssoufi, Valentin D. Ivanov, Gal Matijevic, Florian Niederhofer, Martin Groenewegen, Kenji Bekki, Jonathan Diaz, Joana M. Oliveira, Maria-Rosa L. Cioni, Jacco Th. van Loon
The Magellanic Clouds are a nearby pair of interacting dwarf galaxies and satellites of the Milky Way. Studying their kinematic properties is essential to understanding their origin and dynamical evolution. They have prominent tidal features and the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::59aa3a5873d865bb80d72e14bc498473
https://eprints.keele.ac.uk/8827/1/2006.03163.pdf
https://eprints.keele.ac.uk/8827/1/2006.03163.pdf
Autor:
Cameron P. M. Bell, Vincenzo Ripepi, Valentin D. Ivanov, Maria-Rosa L. Cioni, Florian Niederhofer, Léo Girardi, Stefano Rubele, Gal Matijevic, Kenji Bekki, Richard de Grijs, Jacco Th. van Loon, Dalal El Youssoufi, Joana M. Oliveira, Smitha Subramanian
Publikováno v:
Monthly Notices of the Royal Astronomical Society
The Magellanic Clouds are nearby dwarf irregular galaxies whose morphologies show different properties when traced by different stellar populations, making them an important laboratory for studying galaxy morphologies. We study the morphology of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1973925e9e1ebf9651b43d3f8f1bbe45
Autor:
Cameron P. M. Bell, Florian Niederhofer, Stefano Rubele, Dalal El Youssoufi, Gal Matijevic, Maria-Rosa L. Cioni
Publikováno v:
Proceedings of the International Astronomical Union
The Magellanic Clouds are nearby dwarf irregular galaxies that represent a unique laboratory for studying galaxy interactions. Their morphology and dynamics have been heavily influenced by their mutual interactions as well as with their interaction(s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::874f163381e783f515d7bbe703688c09
Autor:
Vincenzo Ripepi, Laurent Chemin, Roberto Molinaro, Maria-Rosa L Cioni, Kenji Bekki, Gisella Clementini, Richard de Grijs, Giulia De Somma, Dalal El Youssoufi, Léo Girardi, Martin A T Groenewegen, Valentin Ivanov, Marcella Marconi, Paul J McMillan, Jacco Th van Loon
Publikováno v:
Monthly Notices of the Royal Astronomical Society
We employed the {\it VISTA near-infrared $YJK_\mathrm{s}$ survey of the Magellanic System} (VMC), to analyse the $Y,\,J,\,K_\mathrm{s}$ light curves of $\delta$ Cepheid stars (DCEPs) in the Large Magellanic Cloud (LMC). Our sample consists of 4408 ob
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::50e2cc4e03a92a416d9490eee258ec7c