Zobrazeno 1 - 10
of 312
pro vyhledávání: '"Bovino, S"'
Autor:
Solimano, M., González-López, J., Aravena, M., Pampliega, B. Alcalde, Assef, R. J., Béthermin, M., Boquien, M., Bovino, S., Casey, C. M., Cassata, P., da Cunha, E., Davies, R. L., De Looze, I., Ding, X., Díaz-Santos, T., Faisst, A. L., Ferrara, A., Fisher, D. B., Förster-Schreiber, N. M., Fujimoto, S., Ginolfi, M., Gruppioni, C., Guaita, L., Hathi, N., Herrera-Camus, R., Ibar, E., Inami, H., Jones, G. C., Koekemoer, A. M., Lee, L., Li, J., Liu, D., Liu, Z., Molina, J., Ogle, P., Posses, A. C., Pozzi, F., Relaño, M., Riechers, D. A., Romano, M., Spilker, J., Sulzenauer, N., Telikova, K., Vallini, L., Vasan, K. G. C., Veilleux, S., Vergani, D., Villanueva, V., Wang, W., Yan, L., Zamorani, G.
We present new JWST/NIRSpec IFU observations of the J1000+0234 system at $z=4.54$, the dense core of a galaxy protocluster hosting a massive, dusty star forming galaxy (DSFG) with a low luminosity radio counterpart. The new data reveals two extended,
Externí odkaz:
http://arxiv.org/abs/2407.13020
Autor:
Villanueva, V., Herrera-Camus, R., Gonzalez-Lopez, J., Aravena, M., Assef, R. J., Baeza-Garay, Mauricio, Barcos-Muñoz, L., Bovino, S., Bowler, R. A. A., da Cunha, E., De Looze, I., Diaz-Santos, T., Ferrara, A., Foerster-Schreiber, N., Algera, H., Iked, R., Killi, M., Mitsuhashi, I., Naab, T., Relano, M., Spilker, J., Solimano, M., Palla, M., Price, S. H., Posses, A., Tadaki, K., Telikova, K., Übler, H.
We present new $\lambda_{\rm rest}=77$ $\mu$m dust continuum observations from the ALMA of HZ10 (CRISTAL-22), a dusty main-sequence galaxy at $z$=5.66 as part of the [CII] Resolved Ism in STar-forming Alma Large program, CRISTAL. The high angular res
Externí odkaz:
http://arxiv.org/abs/2407.09681
Publikováno v:
A&A 687, A70 (2024)
Cosmic rays regulate the dynamics and the chemical processes in the densest and coldest regions of the ISM. Still, the determination of the cosmic-ray ionisation rate of H$_2$ (${\zeta^{\rm ion}_{{\rm H}_2}}$) is plagued by uncertainties in the adopt
Externí odkaz:
http://arxiv.org/abs/2404.15754
Autor:
Posses, A., Aravena, M., González-López, J., Schreiber, N. M. Förster, Liu, D., Lee, L., Solimano, M., Díaz-Santos, T., Assef, R. J., Barcos-Muñoz, L., Bovino, S., Bowler, R. A. A., Rivera, G. Calistro, da Cunha, E., Davies, R. L., Killi, M., De Looze, I., Ferrara, A., Fisher, D. B., Herrera-Camus, R., Ikeda, R., Lambert, T., Li, J., Lutz, D., Mitsuhashi, I., Palla, M., Relaño, M., Spilker, J., Naab, T., Tadaki, K., Telikova, K., Übler, H., van der Giessen, S., Villanueva, V.
The ALMA [CII] Resolved Ism in STar-forming gALaxies (CRISTAL) survey is a Cycle 8 ALMA Large Programme that studies the cold gas component of high-redshift galaxies. Its sub-arcsecond resolution observations are key to disentangling physical mechani
Externí odkaz:
http://arxiv.org/abs/2403.03379
Autor:
Redaelli, E., Bovino, S., Lupi, A., Grassi, T., Gaete-Espinoza, D., Sabatini, G., Caselli, P.
Cosmic rays (CRs) heavily impact the chemistry and physics of cold and dense star-forming regions. However, characterising their ionisation rate is still challenging from an observational point of view. In the past, a few analytical formulas have bee
Externí odkaz:
http://arxiv.org/abs/2402.10852
Autor:
Redaelli, E., Bovino, S., Sanhueza, P., Morii, K., Sabatini, G., Caselli, P., Giannetti, A., Li, S.
High-mass star formation theories make distinct predictions on the properties of the prestellar seeds of high-mass stars. Observations of the early stages of high-mass star formation can provide crucial constraints, but they are challenging and scarc
Externí odkaz:
http://arxiv.org/abs/2208.01675
Autor:
Henríquez-Brocal, K., Herrera-Camus, R., Tacconi, L., Genzel, R., Bolatto, A., Bovino, S., Demarco, R., Schreiber, N. Förster, Lee, M., Lutz, D., Rubio, M.
We use a combination of new NOrthern Extended Millimeter Array (NOEMA) observations of the pair of [CI] transitions, the CO(7-6) line, and the dust continuum, in addition to ancillary CO(1-0) and CO(3-2) data, to study the molecular gas properties of
Externí odkaz:
http://arxiv.org/abs/2109.01684
Autor:
Sabatini, G., Bovino, S., Giannetti, A., Grassi, T., Brand, J., Schisano, E., Wyrowski, F., Leurini, S., Menten, K. M.
Publikováno v:
A&A 652, A71 (2021)
(Abridged) Understanding the details of the formation process of massive (i.e. M<8-10M$_\odot$) stars is a long-standing problem in astrophysics. [...] We present a method to derive accurate timescales of the different evolutionary phases of the high
Externí odkaz:
http://arxiv.org/abs/2106.00692
In many astrophysical applications, the cost of solving a chemical network represented by a system of ordinary differential equations (ODEs) grows significantly with the size of the network, and can often represent a significant computational bottlen
Externí odkaz:
http://arxiv.org/abs/2104.09516
Autor:
Redaelli, E., Bovino, S., Giannetti, A., Sabatini, G., Caselli, P., Wyrowski, F., Schleicher, D. R. G., Colombo, D.
Publikováno v:
A&A 650, A202 (2021)
Context. The different theoretical models concerning the formation of high-mass stars make distinct predictions regarding their progenitors, i.e. the high-mass prestellar cores. However, so far no conclusive observation of such objects has been made.
Externí odkaz:
http://arxiv.org/abs/2104.06431