Zobrazeno 1 - 10
of 720
pro vyhledávání: '"Sormani M. P."'
Magnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamics
Autor:
Tress, R. G., Sormani, M. C., Girichidis, P., Glover, S. C. O., Klessen, R. S., Smith, R. J., Sobacchi, E., Armillotta, L., Barnes, A. T., Battersby, C., Bogue, K. R. J., Brucy, N., Colzi, L., Federrath, C., García, P., Ginsburg, A., Göller, J., Hatchfield, H P., Henkel, C., Hennebelle, P., Henshaw, J. D., Hirschmann, M., Hu, Y., Kauffmann, J., Kruijssen, J. M. D., Lazarian, A., Lipman, D., Longmore, S. N., Morris, M. R., Nogueras-Lara, F., Petkova, M. A., Pillai, T. G. S., Rivilla, V. M., Sánchez-Monge, Á., Soler, J. D., Whitworth, D., Zhang, Q.
The interstellar medium in the Milky Way's Central Molecular Zone (CMZ) is known to be strongly magnetised, but its large-scale morphology and impact on the gas dynamics are not well understood. We explore the impact and properties of magnetic fields
Externí odkaz:
http://arxiv.org/abs/2403.13048
Autor:
Nieuwmunster, N., Schultheis, M., Sormani, M., Fragkoudi, F., Nogueras-Lara, F., Schödel, R., McMillan, P.
While orbital analysis studies were so far mainly focused on the Galactic halo, it is possible now to do these studies in the heavily obscured region close to the Galactic Centre. We aim to do a detailed orbital analysis of stars located in the nucle
Externí odkaz:
http://arxiv.org/abs/2403.00761
Autor:
Nogueras-Lara, F., Feldmeier-Krause, A., Schödel, R., Sormani, M. C., de Lorenzo-Cáceres, A., Mastrobuono-Battisti, A., Schultheis, M., Neumayer, N., Rich, R. M., Nieuwmunster, N.
Publikováno v:
A&A 680, A75 (2023)
The innermost regions of most galaxies are characterised by the presence of extremely dense nuclear star clusters. Nevertheless, these clusters are not the only stellar component present in galactic nuclei, where larger stellar structures known as nu
Externí odkaz:
http://arxiv.org/abs/2309.07219
Autor:
Veena, V. S., Riquelme, D., Kim, W. -J., Menten, K. M., Schilke, P., Sormani, M. C., Banda-Barragan, W. E., Wyrowski, F., Fuller, G. A., Cheema, A.
Publikováno v:
A&A 674, L15 (2023)
We report the discovery of a velocity coherent, funnel shaped ^13CO emission feature in the Galactic centre (GC) using data from the SEDIGISM survey. The molecular cloud appears as a low velocity structure (V_LSR=[-3.5, +3.5] km/s) with an angular ex
Externí odkaz:
http://arxiv.org/abs/2306.06980
Autor:
Stuber, S. K., Schinnerer, E., Williams, T. G., Querejeta, M., Meidt, S., Emsellem, E., Barnes, A., Klessen, R. S., Leroy, A. K., Neumann, J., Sormani, M. C., Bigiel, F., Chevance, M., Dale, D., Faesi, C., Glover, S. C. O., Grasha, K., Kruijssen, J. M. D., Liu, D., Pan, H., Pety, J., Pinna, F., Saito, T., Usero, A., Watkins, E. J.
Publikováno v:
A&A 676, A113 (2023)
The morphology of a galaxy stems from secular and environmental processes during its evolutionary history. Thus galaxy morphologies have been a long used tool to gain insights on galaxy evolution. We visually classify morphologies on cloud-scales bas
Externí odkaz:
http://arxiv.org/abs/2305.17172
Publikováno v:
A&A 671, L10 (2023)
The nuclear stellar disc (NSD) is a flat dense stellar structure at the heart of the Milky Way. Recent work has shown that analogous structures are common in the nuclei of external spiral galaxies, where there is evidence of an age gradient that indi
Externí odkaz:
http://arxiv.org/abs/2302.02890
Autor:
Anastasopoulou, K., Ponti, G., Sormani, M. C., Locatelli, N., Haberl, F., Morris, M. R., Churazov, E. M., Schödel, R., Maitra, C., Campana, S., Di Teodoro, E. M., Jin, C., Khabibullin, I., Mondal, S., Sasaki, M., Zhang, Y., Zheng, X.
Publikováno v:
A&A 671, A55 (2023)
The diffuse Fe XXV (6.7 keV) line emission observed in the Galactic ridge is widely accepted to be produced by a superposition of a large number of unresolved X-ray point sources. In the very central degrees of our Galaxy, however, the existence of a
Externí odkaz:
http://arxiv.org/abs/2301.04164
Autor:
Maconi, E., Soler, J. D., Reissl, S., Girichidis, P., Klessen, R. S., Hennebelle, P., Molinari, S., Testi, L., Smith, R. J., Sormani, M. C., Teh, J. W., Traficante, A.
We present a study of synthetic observations of polarized dust emission at 353 GHz as seen by an observer within a cavity in the interstellar medium (ISM). The cavity is selected from a magnetohydrodynamic simulation of the local ISM with time-depend
Externí odkaz:
http://arxiv.org/abs/2212.06598
Autor:
Elia, D., Molinari, S., Schisano, E., Soler, J. D., Merello, M., Russeil, D., Veneziani, M., Zavagno, A., Noriega-Crespo, A., Olmi, L., Benedettini, M., Hennebelle, P., Klessen, R. S., Leurini, S., Paladini, R., Pezzuto, S., Traficante, A., Eden, D. J., Martin, P. G., Sormani, M., Coletta, A., Colman, T., Plume, R., Maruccia, Y., Mininni, C., Liu, S. J.
We present a new derivation of the Milky Way's current star formation rate (SFR) based on the data of the Hi-GAL Galactic plane survey. We estimate the distribution of the SFR across the Galactic plane from the star-forming clumps identified in the H
Externí odkaz:
http://arxiv.org/abs/2211.05573
Autor:
Wallace, J., Battersby, C., Mills, E. A. C., Henshaw, J. D., Sormani, M. C., Ginsburg, A., Barnes, A. T., Hatchfield, H. P., Glover, S. C. O., Anderson, L. D.
We report on the discovery of linear filaments observed in CO(1-0) emission for a $\sim2'$ field of view toward the Sgr E star forming region centered at (l,b)=(358.720$^\circ$, 0.011$^\circ$). The Sgr E region is thought to be at the turbulent inter
Externí odkaz:
http://arxiv.org/abs/2209.11781