Zobrazeno 1 - 10
of 5 222
pro vyhledávání: '"Musé I"'
Autor:
Wragg, F., Kamann, S., Saracino, S., Latour, M., Dreizler, S., Martens, S., Seth, A., Vaz, D., van de Ven, G.
Publikováno v:
2024, MNRAS, 535, 781
NGC 5139 ($\omega$ Cen), is the closest candidate of a Nuclear Star Cluster that has been stripped of its host galaxy in the Milky Way. Despite extensive studies through the last decades, many open questions about the cluster remain, including the pr
Externí odkaz:
http://arxiv.org/abs/2411.05680
Edge-on galaxies act as the best laboratories to understand the origin of thin and thick discs in galaxies. Measurement of spatially resolved stellar population properties in such galaxies, particularly age, metallicity and [$\alpha$/Fe], are crucial
Externí odkaz:
http://arxiv.org/abs/2405.17999
Autor:
Izzo, L., Pasquini, L., Aydi, E., Della Valle, M., Gilmozzi, R., Harvey, E. A., Molaro, P., Otulakowska-Hypka, M., Selvelli, P., Thöne, C. C., Williams, R.
Publikováno v:
A&A 686, A72 (2024)
T Pyx is one of the most enigmatic recurrent novae, and it has been proposed as a potential Galactic type-Ia supernova progenitor. Using spatially-resolved data obtained with MUSE, we characterized the geometrical distribution of the material expelle
Externí odkaz:
http://arxiv.org/abs/2312.04277
Akademický článek
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Akademický článek
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Autor:
Della Bruna, Lorenza, Adamo, Angela, Amram, Philippe, Rosolowsky, Erik, Usher, Christopher, Sirressi, Mattia, Schruba, Andreas, Emsellem, Eric, Leroy, Adam, Bik, Arjan, Blair, William P., McLeod, Anna F., Östlin, Göran, Renaud, Florent, Robert, Carmelle, Rousseau-Nepton, Laurie, Smith, Linda J.
Publikováno v:
A&A 660, A77 (2022)
We present a large VLT/MUSE mosaic (3.8 x 3.8 kpc) of the nearby spiral galaxy M83, with a spatial resolution ~20 pc. We obtained the kinematics of the stars and ionised gas, and compared them with molecular gas kinematics from ALMA CO(2-1). We separ
Externí odkaz:
http://arxiv.org/abs/2202.01738
Autor:
De Pontieu, Bart, Testa, Paola, Martinez-Sykora, Juan, Antolin, Patrick, Karampelas, Konstantinos, Hansteen, Viggo, Rempel, Matthias, Cheung, Mark C. M., Reale, Fabio, Danilovic, Sanja, Pagano, Paolo, Polito, Vanessa, De Moortel, Ineke, Nobrega-Siverio, Daniel, Van Doorsselaere, Tom, Petralia, Antonino, Asgari-Targhi, Mahboubeh, Boerner, Paul, Carlsson, Mats, Chintzoglou, Georgios, Daw, Adrian, DeLuca, Ed, Golub, Leon, Matsumoto, Takuma, Ugarte-Urra, Ignacio, McIntosh, Scott, team, the MUSE
The Multi-slit Solar Explorer (MUSE) is a proposed NASA MIDEX mission, currently in Phase A, composed of a multi-slit EUV spectrograph (in three narrow spectral bands centered around 171A, 284A, and 108A) and an EUV context imager (in two narrow pass
Externí odkaz:
http://arxiv.org/abs/2106.15584
Autor:
Roth, Martin M., Jacoby, George H., Ciardullo, Robin, Davis, Brian D., Chase, Owen, Weilbacher, Peter M.
The [O III ] 5007 Planetary Nebula Luminosity Function (PNLF) is an established distance indicator that has been used for more than 30 years to measure the distances of galaxies out to ~15 Mpc. With the advent of the Multi-Unit Spectroscopic Explorer
Externí odkaz:
http://arxiv.org/abs/2105.01982
Autor:
Saracino, S., Kamann, S., Usher, C., Bastian, N., Martocchia, S., Lardo, C., Latour, M., Cabrera-Ziri, I., Dreizler, S., Giesers, B., Husser, T. -O., Kacharov, N., Salaris, M.
Nearly all of the well studied ancient globular clusters (GCs), in the Milky Way and in nearby galaxies, show star-to-star variations in specific elements (e.g., He, C, N, O, Na, Al), known as "multiple populations" (MPs). However, MPs are not restri
Externí odkaz:
http://arxiv.org/abs/2009.03320
Autor:
Della Bruna, Lorenza, Adamo, Angela, Bik, Arjan, Fumagalli, Michele, Walterbos, Rene, Östlin, Göran, Bruzual, Gustavo, Calzetti, Daniela, Charlot, Stephane, Grasha, Kathryn, Smith, Linda J., Thilker, David, Wofford, Aida
Publikováno v:
A&A 652, C6 (2021)
Using MUSE AO data, we probe the ISM in the local spiral galaxy NGC 7793 at a spatial resolution of $\sim$ 10 pc. We identify HII regions and compile a catalogue of supernova remnants (SNRs), planetary nebulae (PNe) and Wolf Rayet stars (WR). We comp
Externí odkaz:
http://arxiv.org/abs/2002.08966