Zobrazeno 1 - 10
of 248
pro vyhledávání: '"Bešlić I"'
Autor:
Querejeta, M., Pety, J., Schruba, A., Leroy, A. K., Herrera, C. N., Chiang, I-D., Meidt, S. E., Rosolowsky, E., Schinnerer, E., Schuster, K., Sun, J., Herrmann, K. A., Barnes, A. T., Beslic, I., Bigiel, F., Cao, Y., Chevance, M., Eibensteiner, C., Emsellem, E., Faesi, C. M., Hughes, A., Kim, J., Klessen, R. S., Kreckel, K., Kruijssen, J. M. D., Liu, D., Neumayer, N., Pan, H. -A., Saito, T., Sandstrom, K., Teng, Y. -S., Usero, A., Williams, T. G., Zakardjian, A.
Publikováno v:
A&A 680, A4 (2023)
We present a new wide-field 10.75 x 10.75 arcmin^2 (~11x11 kpc^2), high-resolution (theta = 3.6" ~ 60 pc) NOEMA CO(1-0) survey of the very nearby (d=3.45 Mpc) spiral galaxy IC 342. The survey spans out to about 1.5 effective radii and covers most of
Externí odkaz:
http://arxiv.org/abs/2310.06501
Autor:
Santa-Maria, M. G., Goicoechea, J. R., Pety, J., Gerin, M., Orkisz, J. H., Petit, F. Le, Einig, L., Palud, P., Magalhaes, V. de Souza, Bešlić, I., Segal, L., Bardeau, S., Bron, E., Chainais, P., Chanussot, J., Gratier, P., Guzmán, V. V., Hughes, A., Languignon, D., Levrier, F., Lis, D. C., Liszt, H. S., Bourlot, J. Le, Oya, Y., Öberg, K., Peretto, N., Roueff, E., Roueff, A., Sievers, A., Thouvenin, P. -A., Yamamoto, S.
Publikováno v:
A&A 679, A4 (2023)
We present 5 deg^2 (~250 pc^2) HCN, HNC, HCO+, and CO J=1-0 maps of the Orion B GMC, complemented with existing wide-field [CI] 492 GHz maps, as well as new pointed observations of rotationally excited HCN, HNC, H13CN, and HN13C lines. We detect anom
Externí odkaz:
http://arxiv.org/abs/2309.03186
Autor:
Jiménez-Donaire, M. J., Usero, A., Bešlić, I., Tafalla, M., Chacón-Tanarro, A., Salomé, Q., Eibensteiner, C., García-Rodríguez, A., Hacar, A., Barnes, A. T., Bigiel, F., Chevance, M., Colombo, D., Dale, D. A., Davis, T. A., Glover, S. C. O., Kauffmann, J., Klessen, R. S., Leroy, A. K., Neumann, L., Pan, H., Pety, J., Querejeta, M., Saito, T., Schinnerer, E., Stuber, S., Williams, T. G.
Publikováno v:
A&A 676, L11 (2023)
Nitrogen hydrides such as NH$_3$ and N$_2$H$^+$ are widely used by Galactic observers to trace the cold dense regions of the interstellar medium. In external galaxies, because of limited sensitivity, HCN has become the most common tracer of dense gas
Externí odkaz:
http://arxiv.org/abs/2308.01342
Autor:
Barnes, A. T., Glover, S. C. O., Kreckel, K., Ostriker, E. C., Bigiel, F., Belfiore, F., Bešlić, I., Blanc, G. A., Chevance, M., Dale, D. A., Egorov, O., Eibensteiner, C., Emsellem, E., Grasha, K., Groves, B. A., Klessen, R. S., Kruijssen, J. M. D., Leroy, A. K., Longmore, S. N., Lopez, L., McElroy, R., Meidt, S. E., Murphy, E. J., Rosolowsky, E., Saito, T., Santoro, F., Schinnerer, E., Schruba, A., Sun, J., Watkins, E. J., Williams, T. G.
The feedback from young stars (i.e. pre-supernova) is thought to play a crucial role in molecular cloud destruction. In this paper, we assess the feedback mechanisms acting within a sample of 5810 HII regions identified from the PHANGS-MUSE survey of
Externí odkaz:
http://arxiv.org/abs/2110.05492
Autor:
Querejeta, M., Schinnerer, E., Meidt, S., Sun, J., Leroy, A. K., Emsellem, E., Klessen, R. S., Munoz-Mateos, J. C., Salo, H., Laurikainen, E., Beslic, I., Blanc, G. A., Chevance, M., Dale, D. A., Eibensteiner, C., Faesi, C., Garcia-Rodriguez, A., Glover, S. C. O., Grasha, K., Henshaw, J., Herrera, C., Hughes, A., Kreckel, K., Kruijssen, J. M. D., Liu, D., Murphy, E. J., Pan, H. -A., Pety, J., Razza, A., Rosolowsky, E., Saito, T., Schruba, A., Usero, A., Watkins, E. J., Williams, T. G.
Publikováno v:
A&A 656, A133 (2021)
We identify stellar structures in the PHANGS sample of 74 nearby galaxies and construct morphological masks of sub-galactic environments based on Spitzer 3.6 micron images. At the simplest level, we distinguish centres, bars, spiral arms, interarm an
Externí odkaz:
http://arxiv.org/abs/2109.04491
Autor:
Bešlić, I., Barnes, A. T., Bigiel, F., Puschnig, J., Pety, J., Contreras, C. Herrera, Leroy, A. K., Usero, A., Schinnerer, E., Meidt, S. E., Emsellem, E., Hughes, A., Faesi, C., Kreckel, K., Belfiore, F. M. C., Chevance, M., Brok, J. S. den, Eibensteiner, C., Glover, S. C. O., Grasha, K., Jimenez-Donaire, M. J., Klessen, R. S., Kruijssen, J. M. D., Liu, D., Pessa, I., Querejeta, M., Rosolowsky, E., Saito, T., Santoro, F., Schruba, A., Sormani, M. C., Williams, T. G.
It is still poorly constrained how the densest phase of the interstellar medium varies across galactic environment. A large observing time is required to recover significant emission from dense molecular gas at high spatial resolution, and to cover a
Externí odkaz:
http://arxiv.org/abs/2106.09742
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Autor:
Belis, C.A., Pernigotti, D., Pirovano, G., Favez, O., Jaffrezo, J.L., Kuenen, J., Denier van Der Gon, H., Reizer, M., Riffault, V., Alleman, L.Y., Almeida, M., Amato, F., Angyal, A., Argyropoulos, G., Bande, S., Beslic, I., Besombes, J.-L., Bove, M.C., Brotto, P., Calori, G., Cesari, D., Colombi, C., Contini, D., De Gennaro, G., Di Gilio, A., Diapouli, E., El Haddad, I., Elbern, H., Eleftheriadis, K., Ferreira, J., Vivanco, M. Garcia, Gilardoni, S., Golly, B., Hellebust, S., Hopke, P.K., Izadmanesh, Y., Jorquera, H., Krajsek, K., Kranenburg, R., Lazzeri, P., Lenartz, F., Lucarelli, F., Maciejewska, K., Manders, A., Manousakas, M., Masiol, M., Mircea, M., Mooibroek, D., Nava, S., Oliveira, D., Paglione, M., Pandolfi, M., Perrone, M., Petralia, E., Pietrodangelo, A., Pillon, S., Pokorna, P., Prati, P., Salameh, D., Samara, C., Samek, L., Saraga, D., Sauvage, S., Schaap, M., Scotto, F., Sega, K., Siour, G., Tauler, R., Valli, G., Vecchi, R., Venturini, E., Vestenius, M., Waked, A., Yubero, E.
Publikováno v:
In Atmospheric Environment: X January 2020 5
Ground state of weakly bound dimers and trimers with a radius extending well into the classically forbidden region is explored, with the goal to test the predicted universality of quantum halo states. The focus of the study are molecules consisting o
Externí odkaz:
http://arxiv.org/abs/1411.6347
The ground state properties of spin-polarized deuterium (D$\downarrow$) at zero temperature are obtained by means of the diffusion Monte Carlo calculations within the fixed-node approximation. Three D$\downarrow$ species have been investigated (D$\do
Externí odkaz:
http://arxiv.org/abs/1210.7945