Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Battersby, Cara D."'
Autor:
Cotera, Angela S., Hankins, Matthew J., Bally, John, Barnes, Ashley T., Battersby, Cara D., Hatchfield, H Perry, Herter, Terry L., Lau, Ryan M., Longmore, Steven N., Mills, Elisabeth A. C., Morris, Mark R., Radomski, James T., Simpson, Janet P., Stephens, Zachary, Walker, Daniel L.
The central regions of the Milky Way constitute a unique laboratory for a wide swath of astrophysical studies, consequently the inner $\sim$400 pc has been the target of numerous large surveys at all accessible wavelengths. In this paper we present a
Externí odkaz:
http://arxiv.org/abs/2407.08054
Autor:
Ginsburg, Adam, Barnes, Ashley T., Battersby, Cara D., Bulatek, Alyssa, Gramze, Savannah, Henshaw, Jonathan D., Jeff, Desmond, Lu, Xing, Mills, E. A. C., Walker, Daniel L.
We report JWST NIRCam observations of G0.253+0.016, the molecular cloud in the Central Molecular Zone known as The Brick, with the F182M, F187N, F212N, F410M, F405N, and F466N filters. We catalog 56,146 stars detected in all 6 filters using the crowd
Externí odkaz:
http://arxiv.org/abs/2308.16050
Autor:
Sormani, Mattia C., Tress, Robin G., Glover, Simon C. O., Klessen, Ralf S., Battersby, Cara D., Clark, Paul C., Hatchfield, H Perry, Smith, Rowan J.
The Milky Way's central molecular zone (CMZ) has emerged in recent years as a unique laboratory for the study of star formation. Here we use the simulations presented in Tress et al. 2020 to investigate star formation in the CMZ. These simulations re
Externí odkaz:
http://arxiv.org/abs/2004.06731
Autor:
Tress, Robin G., Sormani, Mattia C., Glover, Simon C. O., Klessen, Ralf S., Battersby, Cara D., Clark, Paul C., Hatchfield, H Perry, Smith, Rowan J.
We use hydrodynamical simulations to study the Milky Way's central molecular zone (CMZ). The simulations include a non-equilibrium chemical network, the gas self-gravity, star formation and supernova feedback. We resolve the structure of the interste
Externí odkaz:
http://arxiv.org/abs/2004.06724
Autor:
Sormani, Mattia C., Tress, Robin G., Glover, Simon C. O., Klessen, Ralf S., Barnes, Ashley T., Battersby, Cara D., Clark, Paul C., Hatchfield, H Perry, Smith, Rowan J.
Observations of molecular gas near the Galactic centre ($| l | < 10^\circ$, $| b | < 1^\circ$) reveal the presence of a distinct population of enigmatic compact clouds which are characterised by extreme velocity dispersions ($\Delta v > 100\, \rm km/
Externí odkaz:
http://arxiv.org/abs/1906.10129
Autor:
Ginsburg, Adam, Mills, Elisabeth A. C., Battersby, Cara D., Longmore, Steven N., Kruijssen, J. M. Diederik
The closest galaxy center, our own Central Molecular Zone (CMZ; the central 500 pc of the Milky Way), is a powerful laboratory for studying the secular processes that shape galaxies across cosmic time, from large-scale gas flows and star formation to
Externí odkaz:
http://arxiv.org/abs/1903.04525
Autor:
Ginsburg, Adam, Goss, W. M., Goddi, Ciriaco, Galván-Madrid, Roberto, Dale, James E., Bally, John, Battersby, Cara D., Youngblood, Allison, Sankrit, Ravi, Smith, Rowan, Darling, Jeremy, Kruijssen, J. M. Diederik, Liu, Hauyu Baobab
Publikováno v:
A&A 595, A27 (2016)
We present new JVLA observations of the high-mass cluster-forming region W51A from 2 to 16 GHz with resolution ${\theta}_{fwhm} \approx$ 0.3 - 0.5". The data reveal a wealth of observational results: (1) Currently-forming, very massive (proto-O) star
Externí odkaz:
http://arxiv.org/abs/1605.09402
Autor:
Sormani, Mattia C, Treß, Robin G, Glover, Simon C O, Klessen, Ralf S, Barnes, Ashley T, Battersby, Cara D, Clark, Paul C, Hatchfield, H Perry, Smith, Rowan J
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Oct2019, Vol. 488 Issue 4, p4663-4673, 11p
