Zobrazeno 1 - 10
of 7 373
pro vyhledávání: '"Combès, A."'
Autor:
Poitevineau, R., Combes, F., Garcia-Burillo, S., Cornu, D., Herrero, A. Alonso, Almeida, C. Ramos, Audibert, A., Bellocchi, E., Boorman, P. G., Bunker, A. J., Davies, R., Díaz-Santos, T., García-Bernete, I., García-Lorenzo, B., González-Martín, O., Hicks, E. K. S., Hönig, S. F., Hunt, L. K., Imanishi, M., Pereira-Santaella, M., Ricci, C., Rigopoulou, D., Rosario, D. J., Rouan, D., Martin, M. Villar, Ward, M.
The detailed feeding and feedback mechanisms of Active Galactic Nuclei (AGN) are not yet well known. For low-luminosity and obscured AGN, as well as late-type galaxies, determining the central black hole (BH) masses is challenging. Our goal with the
Externí odkaz:
http://arxiv.org/abs/2411.18200
Autor:
Fuller, Lindsay, Lopez-Rodriguez, Enrique, Garcia-Bernete, Ismael, Almeida, Cristina Ramos, Alonso-Herrero, Almudena, Packham, Chris, Zhang, Lulu, Leist, Mason, Levenson, Nancy, Imanishi, Masa, Hoenig, Sebastian, Stalevski, Marko, Ricci, Claudio, Hicks, Erin, Bellocchi, Enrica, Combes, Francoise, Davies, Ric, Burillo, Santiago Garcia, GonzalezMartin, Omaira, TakumaIzumi, Labiano, Alvaro, Santaella, Miguel Pereira, Rigopoulou, Dimitra, Rosario, David, Rouan, Daniel, Shimizu, Taro, Ward, Martin
We present a 19.7 - 214 $\mu$m imaging atlas of local (4 - 181 Mpc; median 43 Mpc) active galactic nuclei (AGN) observed with FORCAST and HAWC+ on board the SOFIA telescope with angular resolutions ~ 3"- 20". This atlas comprises 22 Seyferts (17 Type
Externí odkaz:
http://arxiv.org/abs/2411.18738
The Andromeda galaxy (M31) is the most nearby giant spiral galaxy, an opportunity to study with high resolution dynamical phenomena occurring in nuclear disks and bulges, able to explain star formation quenching, and galaxy evolution through collisio
Externí odkaz:
http://arxiv.org/abs/2411.18460
Autor:
Esparza-Arredondo, D., Almeida, C. Ramos, Audibert, A., Pereira-Santaella, M., García-Bernete, I., García-Burillo, S., Shimizu, T., Davies, R., Muñoz, L. Hermosa, Alonso-Herrero, A., Combes, F., Speranza, G., Zhang, L., Campbell, S., Bellocchi, E., Bunker, A. J., Díaz-Santos, T., García-Lorenzo, B., González-Martín, O., Hicks, E. K. S., Labiano, A., Levenson, N. A., Ricci, C., Rosario, D., Hoenig, S., Packham, C., Stalevski, M., Fuller, L., Izumi, T., López-Rodríguez, E., Rigopoulou, D., Rouan, D., Ward, M.
Understanding the processes that drive the morphology and kinematics of molecular gas in galaxies is crucial for comprehending star formation and, ultimately, galaxy evolution. Using data obtained with the James Webb Space Telescope (JWST) and the At
Externí odkaz:
http://arxiv.org/abs/2411.12398
Autor:
Veronese, S., de Blok, W. J. G., Healy, J., Kleiner, D., Marasco, A., Maccagni, F. M., Kamphuis, P., Brinks, E., Holwerda, B. W., Zabel, N., Chemin, L., Adams, E. A. K., Kurapati, S., Sorgho, A., Spekkens, K., Combes, F., Pisano, D. J., Walter, F., Amram, P., Bigiel, F., Wong, O. I., Athanassoula, E.
The observed star formation rates of galaxies in the Local Universe suggests that they are replenishing their gas reservoir across cosmic time. Cosmological simulations predict that this accretion of fresh gas can occur in a hot or a cold mode, yet t
Externí odkaz:
http://arxiv.org/abs/2411.11584
Autor:
Gil, D. Fernández, Hodgson, J. A., L'Huillier, B., Asorey, J., Saulder, C., Finner, K., Jee, M. J., Parkinson, D., Combes, F.
The relationship between galaxies and their supermassive black holes (SMBHs) is an area of active research. One way to investigate this is to compare parsec-scale jets formed by SMBHs with the projected shape of their kiloparsec-scale host galaxies.
Externí odkaz:
http://arxiv.org/abs/2411.09099
Autor:
Fraser-McKelvie, A., van de Sande, J., Gadotti, D. A., Emsellem, E., Brown, T., Fisher, D. B., Martig, M., Bureau, M., Gerhard, O., Battisti, A. J., Bland-Hawthorn, J., Catinella, B., Combes, F., Cortese, L., Croom, S. M., Davis, T. A., Falcón-Barroso, J., Fragkoudi, F., Freeman, K. C., Hayden, M. R., McDermid, R., Ciraulo, B. Mazzilli, Mendel, J. T., Pinna, F., Poci, A., Rutherford, T. H., de Sá-Freitas, C., Silva-Lima, L. A., Valenzuela, L. M., van de Ven, G., Wang, Z., Watts, A. B.
The vertical evolution of galactic discs is governed by the sub-structures within them. We examine the diversity of kinematic sub-structure present in the first 12 galaxies observed from the GECKOS survey, a VLT/MUSE large programme providing a syste
Externí odkaz:
http://arxiv.org/abs/2411.03430
Autor:
Conger, Kim, Rudnick, Gregory, Finn, Rose A., Castignani, Gianluca, Moustakas, John, Vulcani, Benedetta, Zakharova, Daria, Xie, Lizhi, Combes, Francoise, Jablonka, Pascale, Bahé, Yannick, De Lucia, Gabriella, Desai, Vandana, Koopmann, Rebecca A., Norman, Dara, Townsend, Melinda, Zaritsky, Dennis
Recent theoretical work and targeted observational studies suggest that filaments are sites of galaxy preprocessing. The aim of the WISESize project is to directly probe galaxies over the full range of environments to quantify and characterize extrin
Externí odkaz:
http://arxiv.org/abs/2411.02352
Permutation puzzles, such as the Rubik's cube and the 15 puzzle, are enjoyed by the general public and mathematicians alike. Here we introduce quantum versions of permutation puzzles where the pieces of the puzzles are replaced with indistinguishable
Externí odkaz:
http://arxiv.org/abs/2410.22287
Autor:
Venkattu, Deepika, Lundqvist, Peter, Torres, Miguel Pérez, Bonnassieux, Etienne, Tasse, Cyril, Melchior, Anne-Laure, Combes, Francoise
We present the first LOFAR image of the centre of M31 at a frequency of 150 MHz. We clearly detect three supernova remnants, which, along with archival VLA data at 3 GHz and other published radio and X-ray data allows us to characterize them in detai
Externí odkaz:
http://arxiv.org/abs/2410.22073