Zobrazeno 1 - 10
of 2 285
pro vyhledávání: '"Rosolowsky E"'
Autor:
King, S. M., Moore, T. J. T., Henshaw, J. D., Longmore, S. N., Eden, D. J., Rigby, A. J., Rosolowsky, E., Tahani, K., Su, Y., Yiping, A., Tang, X., Ragan, S., Liu, T., Kuan, Y. -J., Rani, R.
We present the initial data for the ($J = 3 \to 2$) transition of $^{13}$CO obtained from the Central Molecular Zone (CMZ) of the Milky Way as part of the CO Heterodyne Inner Milky Way Plane Survey 2 (CHIMPS2). Covering $359^\circ \leq l \leq 1^\circ
Externí odkaz:
http://arxiv.org/abs/2408.11548
Autor:
Brok, J. S. den, Leroy, A. K., Usero, A., Schinnerer, E., Rosolowsky, E., Koch, E. W., Querejeta, M., Liu, D., Bigiel, F., Barnes, A. T., Chevance, M., Colombo, D., Dale, D. A., Glover, S. C. O., Jimenez-Donaire, M. J., Teng, Y. -H., Williams, T. G.
The low-$J$ rotational transitions of $^{12}$CO are commonly used to trace the distribution of molecular gas in galaxies. Their ratios are sensitive to excitation and physical conditions in the molecular gas. Spatially resolved studies of CO ratios a
Externí odkaz:
http://arxiv.org/abs/2310.18407
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:
Pandhi, A., Friesen, R. K., Fissel, L., Pineda, J. E., Caselli, P., Chen, M. C-Y., Di Francesco, J., Ginsburg, A., Kirk, H., Myers, P. C., Offner, S. S. R., Punanova, A., Quan, F., Redaelli, E., Rosolowsky, E., Scibelli, S., Seo, Y. M., Shirley, Y.
Studies of dense core morphologies and their orientations with respect to gas flows and the local magnetic field have been limited to only a small sample of cores with spectroscopic data. Leveraging the Green Bank Ammonia Survey alongside existing su
Externí odkaz:
http://arxiv.org/abs/2307.13022
Autor:
Pessa, I., Schinnerer, E., Sanchez-Blazquez, P., Belfiore, F., Groves, B., Emsellem, E., Neumann, J., Leroy, A. K., Bigiel, F., Chevance, M., Dale, D. A., Glover, S. C. O., Grasha, K., Klessen, R. S., Kreckel, K., Kruijssen, J. M. D., Pinna, F., Querejeta, M., Rosolowsky, E., Williams, T. G.
Publikováno v:
A&A 673, A147 (2023)
Analyzing resolved stellar populations across the disk of a galaxy can provide unique insights into how that galaxy assembled its stellar mass over its lifetime. Previous work at ~1 kpc resolution has already revealed common features in the mass buil
Externí odkaz:
http://arxiv.org/abs/2303.13676
Autor:
Kalinova, V., Colombo, D., Sánchez, S. F., Rosolowsky, E., Kodaira, K., García-Benito, R., Meidt, S. E., Davis, T. A., Romeo, A. B., Yu, S. -Y., Delgado, R. González, Lacerda, E. A. D.
Publikováno v:
A&A 665, A90 (2022)
It has been suggested that the gravitational potential can have a significant role in suppressing the star formation in the nearby galaxies. To establish observational constrains on this scenario, we investigate the connection between the dynamics, t
Externí odkaz:
http://arxiv.org/abs/2207.03872
Autor:
Pessa, I., Schinnerer, E., Leroy, A., Koch, E., Rosolowsky, E., Williams, T., Pan, H. -A., Schruba, A., Usero, A., Belfiore, F., Bigiel, F., Blanc, G., Chevance, M., Dale, D., Emsellem, E., Gensior, J., Glover, S., Grasha, K., Groves, B., Klessen, R., Kreckel, K., Kruijssen, J. M. D., Liu, D., Meidt, S. E., Pety, J., Querejeta, M., Saito, T., Sanchez-Blazquez, P., Watkins, E. J.
Publikováno v:
A&A 663, A61 (2022)
There exists some consensus that stellar mass surface density ($\Sigma_{*}$) and molecular gas mass surface density ($\Sigma_{\rm mol}$) are the main quantities responsible for locally setting the star formation rate. This regulation is inferred from
Externí odkaz:
http://arxiv.org/abs/2203.11971
Autor:
Ginsburg, A., Csengeri, T., Galván-Madrid, R., Cunningham, N., Álvarez-Gutiérrez, R. H., Baug, T., Bonfand, M., Bontemps, S., Busquet, G., Díaz-González, D. J., Fernández-López, M., Guzmán, A., Herpin, F., Liu, H., López-Sepulcre, A., Louvet, F., Maud, L., Motte, F., Nakamura, F., Nony, T., Olguin, F. A., Pouteau, Y., Sanhueza, P., Stutz, A. M., Towner, A. P. M., Armante, M., Battersby, C., Bronfman, L., Braine, J., Brouillet, N., Chapillon, E., Di Francesco, J., Gusdorf, A., Izumi, N., Joncour, I., Lu, X., Men'shchikov, A., Menten, K. M., Moraux, E., Molet, J., Mundy, L., Luong, Q. Nguyen, Reyes-Reyes, S. D., Robitaille, J., Rosolowsky, E., Sandoval-Garrido, N. A., Svoboda, B., Tatematsu, K., Walker, D. L., Whitworth, A., Wu, B., Wyrowski, F.
Publikováno v:
A&A 662, A9 (2022)
We present the first data release of the ALMA-IMF Large Program, which covers the 12m-array continuum calibration and imaging. The ALMA-IMF Large Program is a survey of fifteen dense molecular cloud regions spanning a range of evolutionary stages tha
Externí odkaz:
http://arxiv.org/abs/2112.08183
Autor:
Motte, F., Bontemps, S., Csengeri, T., Pouteau, Y., Louvet, F., Stutz, A. M., Cunningham, N., López-Sepulcre, A., Brouillet, N., Galván-Madrid, R., Ginsburg, A., Maud, L., Men'shchikov, A., Nakamura, F., Nony, T., Sanhueza, P., Álvarez-Gutiérrez, R. H., Armante, M., Baug, T., Bonfand, M., Busquet, G., Chapillon, E., Díaz-González, D., Fernández-López, M., Guzmán, A. E., Herpin, F., Liu, H. -L., Olguin, F., Towner, A. P. M., Bally, J., Battersby, C., Braine, J., Bronfman, L., Chen, H. -R. V., Dell'Ova, P., Di Francesco, J., González, M., Gusdorf, A., Hennebelle, P., Izumi, N., Joncour, I., Lee, Y. -N., Lefloch, B., Lesaffre, P., Lu, X., Menten, K. M., Mignon-Risse, R., Molet, J., Moraux, E., Mundy, L., Luong, Q. Nguyen, Reyes, N., Reyes, S. D. Reyes, Robitaille, J. -F., Rosolowsky, E., Sandoval-Garrido, N. A., Schuller, F., Svoboda, B., Tatematsu, K., Thomasson, B., Walker, D., Wu, B., Whitworth, A. P., Wyrowski, F.
Publikováno v:
A&A 662, A8 (2022)
The ALMA-IMF Large Program imaged a total noncontiguous area of 53pc2, covering 15 extreme, nearby protoclusters of the Milky Way. They were selected to span relevant early protocluster evolutionary stages. Our 1.3mm and 3mm observations provide cont
Externí odkaz:
http://arxiv.org/abs/2112.08182
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