Zobrazeno 1 - 10
of 51 421
pro vyhledávání: '"Battersby A"'
Serve sophisticated, satisfying food--regardless of kitchen's size or scope--with recipes and advice from award-winning chefs Joseph Ogrodnek and Walker Stern of Brooklyn's Battersby and Dover fame. Ogrodnek and Stern cook stellar meals in their rest
Autor:
CANAVAN, TONY
Publikováno v:
Books Ireland, 2019 Mar 01(384), 16-17.
Externí odkaz:
https://www.jstor.org/stable/26852868
Autor:
Trzyna, Thomas, author
Publikováno v:
Karl Popper and Literary Theory: Critical Rationalism as a Philosophy of Literature. 22:46-73
Autor:
Battersby, John, Battersby, Margaret
Publikováno v:
BMJ: British Medical Journal, 2010 Jun . 340(7761), 1418-1418.
Externí odkaz:
https://www.jstor.org/stable/20734641
Autor:
Battersby, Cara, Walker, Daniel L., Barnes, Ashley, Ginsburg, Adam, Lipman, Dani, Alboslani, Danya, Hatchfield, H Perry, Bally, John, Glover, Simon C. O., Henshaw, Jonathan D., Immer, Katharina, Klessen, Ralf S., Longmore, Steven N., Mills, Elisabeth A. C., Molinari, Sergio, Smith, Rowan, Sormani, Mattia C., Tress, Robin G., Zhang, Qizhou
The Central Molecular Zone (CMZ) is the way station at the heart of our Milky Way Galaxy, connecting gas flowing in from Galactic scales with the central nucleus. Key open questions remain about its 3-D structure, star formation properties, and role
Externí odkaz:
http://arxiv.org/abs/2410.17332
Autor:
Battersby, Cara, Walker, Daniel L., Barnes, Ashley, Ginsburg, Adam, Lipman, Dani, Alboslani, Danya, Hatchfield, H Perry, Bally, John, Glover, Simon C. O., Henshaw, Jonathan D., Immer, Katharina, Klessen, Ralf S., Longmore, Steven N., Mills, Elisabeth A. C., Molinari, Sergio, Smith, Rowan, Sormani, Mattia C., Tress, Robin G., Zhang, Qizhou
The Central Molecular Zone (CMZ) is the largest reservoir of dense molecular gas in the Galaxy and is heavily obscured in the optical and near-IR. We present an overview of the far-IR dust continuum, where the molecular clouds are revealed, provided
Externí odkaz:
http://arxiv.org/abs/2410.17334
Autor:
Lipman, Dani, Battersby, Cara, Walker, Daniel L., Sormani, Mattia C., Bally, John, Barnes, Ashley, Ginsburg, Adam, Glover, Simon C. O., Henshaw, Jonathan D., Hatchfield, H Perry, Immer, Katharina, Klessen, Ralf S., Longmore, Steven N., Mills, Elisabeth A. C., Smith, Rowan, Tress, R. G., Alboslani, Danya, Zhang, Qizhou
A comprehensive 3-D model of the central 300 pc of the Milky Way, the Central Molecular Zone (CMZ) is of fundamental importance in understanding energy cycles in galactic nuclei, since the 3-D structure influences the location and intensity of star f
Externí odkaz:
http://arxiv.org/abs/2410.17321
Autor:
Walker, Daniel L., Battersby, Cara, Lipman, Dani, Sormani, Mattia C., Ginsburg, Adam, Glover, Simon C. O., Henshaw, Jonathan D., Longmore, Steven N., Klessen, Ralf S., Immer, Katharina, Alboslani, Danya, Bally, John, Barnes, Ashley, Hatchfield, H Perry, Mills, Elisabeth A. C., Smith, Rowan, Tress, Robin G., Zhang, Qizhou
The Milky Way's Central Molecular Zone (CMZ) is the largest concentration of dense molecular gas in the Galaxy, the structure of which is shaped by the complex interplay between Galactic-scale dynamics and extreme physical conditions. Understanding t
Externí odkaz:
http://arxiv.org/abs/2410.17320
Autor:
Nonhebel, M., Barnes, A. T., Immer, K., Armijos-Abendaño, J., Bally, J., Battersby, C., Burton, M. G., Butterfield, N., Colzi, L., García, P., Ginsburg, A., Henshaw, J. D., Hu, Y., Jiménez-Serra, I., Klessen, R. S., Kruijssen, J. M. D., Liang, F. -H., Longmore, S. N., Lu, X., Martín, S., Mills, E. A. C., Nogueras-Lara, F., Petkova, M. A., Pineda, J. E., Rivilla, V. M., Sánchez-Monge, Á., Santa-Maria, M. G., Smith, H. A., Sofue, Y., Sormani, M. C., Tolls, V., Walker, D. L., Wallace, J., Wang, Q. D., Williams, G. M., Xu, F. -W.
The Milky Way's Central Molecular Zone (CMZ) differs dramatically from our local solar neighbourhood, both in the extreme interstellar medium conditions it exhibits (e.g. high gas, stellar, and feedback density) and in the strong dynamics at play (e.
Externí odkaz:
http://arxiv.org/abs/2409.12185
Autor:
Wells, M. R. A., Beuther, H., Molinari, S., Schilke, P., Battersby, C., Ho, P., Sánchez-Monge, Á., Jones, B., Scheuck, M. B., Syed, J., Gieser, C., Kuiper, R., Elia, D., Coletta, A., Traficante, A., Wallace, J., Rigby, A. J., Klessen, R. S., Zhang, Q., Walch, S., Beltrán, M. T., Tang, Y., Fuller, G. A., Lis, D. C., Möller, T., van der Tak, F., Klaassen, P. D., Clarke, S. D., Moscadelli, L., Mininni, C., Zinnecker, H., Maruccia, Y., Pezzuto, S., Benedettini, M., Soler, J. D., Brogan, C. L., Avison, A., Sanhueza, P., Schisano, E., Liu, T., Fontani, F., Rygl, K. L. J., Wyrowski, F., Bally, J., Walker, D. L., Ahmadi, A., Koch, P., Merello, M., Law, C. Y., Testi, L.
Publikováno v:
A&A 690, A185 (2024)
We use data from the ALMA Evolutionary Study of High Mass Protocluster Formation in the Galaxy (ALMAGAL) survey to study 100 ALMAGAL regions at $\sim$ 1 arsecond resolution located between $\sim$ 2 and 6 kpc distance. Using ALMAGAL $\sim$ 1.3mm line
Externí odkaz:
http://arxiv.org/abs/2408.08299