Zobrazeno 1 - 10
of 127
pro vyhledávání: '"Henshaw, J D"'
Autor:
Cosentino, G., Jiménez-Serra, I., Barnes, A. T., Tan, J. C., Fontani, F., Caselli, P., Henshaw, J. D., Law, C. Y., Viti, S., Fedriani, R., Hsu, C. -J., Gorai, P., Zeng, S., De Simone, M.
How Supernova Remnant (SNR) shocks impact nearby molecular clouds is still poorly observationally constrained. It is unclear if SNRs can positively or negatively affect clouds star formation potential. We have studied the dense gas morphology and kin
Externí odkaz:
http://arxiv.org/abs/2411.16459
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:
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 $359^\circ \leq l \leq 1^\circ
Externí odkaz:
http://arxiv.org/abs/2408.11548
Autor:
Zhang, S., Cyganowski, C. J., Henshaw, J. D., Brogan, C. L., Hunter, T. R., Friesen, R., Bonnell, I. A., Viti, S.
We present deep, sub-arcsecond ($\sim$2000 AU) resolution ALMA 0.82 mm observations of the former high-mass prestellar core candidate G11.92-0.61 MM2, recently shown to be an $\sim$500 AU-separation protobinary. Our observations show that G11.92-0.61
Externí odkaz:
http://arxiv.org/abs/2407.19552
Magnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamics
Autor:
Tress, R. G., Sormani, M. C., Girichidis, P., Glover, S. C. O., Klessen, R. S., Smith, R. J., Sobacchi, E., Armillotta, L., Barnes, A. T., Battersby, C., Bogue, K. R. J., Brucy, N., Colzi, L., Federrath, C., García, P., Ginsburg, A., Göller, J., Hatchfield, H P., Henkel, C., Hennebelle, P., Henshaw, J. D., Hirschmann, M., Hu, Y., Kauffmann, J., Kruijssen, J. M. D., Lazarian, A., Lipman, D., Longmore, S. N., Morris, M. R., Nogueras-Lara, F., Petkova, M. A., Pillai, T. G. S., Rivilla, V. M., Sánchez-Monge, Á., Soler, J. D., Whitworth, D., Zhang, Q.
Publikováno v:
A&A 691, A303 (2024)
The interstellar medium in the Milky Way's Central Molecular Zone (CMZ) is known to be strongly magnetised, but its large-scale morphology and impact on the gas dynamics are not well understood. We explore the impact and properties of magnetic fields
Externí odkaz:
http://arxiv.org/abs/2403.13048
Autor:
Cosentino, G., Tan, J. C., Jiménez-Serra, I., Fontani, F., Caselli, P., Henshaw, J. D., Barnes, A. T., Law, C. -Y., Viti, S., Fedriani, R., Hsu, C. -J., Gorai, P., Zeng, S.
Publikováno v:
A&A 675, A190 (2023)
Supernova remnants (SNRs) may regulate star formation in galaxies. For example, SNR-driven shocks may form new molecular gas or compress pre-existing clouds and trigger the formation of new stars. To test this scenario, we measure the deuteration of
Externí odkaz:
http://arxiv.org/abs/2306.02877
Autor:
Barnes, A. T., Liu, J., Zhang, Q., Tan, J. C., Bigiel, F., Caselli, P., Cosentino, G., Fontani, F., Henshaw, J. D., Jiménez-Serra, I., Kalb, D-S., Law, C. Y., Longmore, S. N., Parker, R. J., Pineda, J. E., Sánchez-Monge, A., Lim, W., Wang, K.
Context: Core accretion models of massive star formation require the existence of massive, starless cores within molecular clouds. Yet, only a small number of candidates for such truly massive, monolithic cores are currently known. Aims: Here we anal
Externí odkaz:
http://arxiv.org/abs/2303.15499
Autor:
Wallace, J., Battersby, C., Mills, E. A. C., Henshaw, J. D., Sormani, M. C., Ginsburg, A., Barnes, A. T., Hatchfield, H. P., Glover, S. C. O., Anderson, L. D.
We report on the discovery of linear filaments observed in CO(1-0) emission for a $\sim2'$ field of view toward the Sgr E star forming region centered at (l,b)=(358.720$^\circ$, 0.011$^\circ$). The Sgr E region is thought to be at the turbulent inter
Externí odkaz:
http://arxiv.org/abs/2209.11781
Autor:
Cosentino, G., Jiménez-Serra, I., Tan, J. C., Henshaw, J. D., Barnes, A. T., Law, C. -Y., Zeng, S., Fontani, F., Caselli, P., Viti, S., Zahorecz, S., Rico-Villas, F., Megías, A., Miceli, M., Orlando, S., Ustamujic, S., Greco, E., Peres, G., Bocchino, F., Fedriani, R., Gorai, P., Testi, L., Martín-Pintado, J.
Supernova remnants (SNRs) contribute to regulate the star formation efficiency and evolution of galaxies. As they expand into the interstellar medium (ISM), they transfer vast amounts of energy and momentum that displace, compress and heat the surrou
Externí odkaz:
http://arxiv.org/abs/2201.03008
Autor:
Syed, J., Soler, J. D., Beuther, H., Wang, Y., Suri, S., Henshaw, J. D., Riener, M., Bialy, S., Kh., S. Rezaei, Stil, J. M., Goldsmith, P. F., Rugel, M. R., Glover, S. C. O., Klessen, R. S., Kerp, J., Urquhart, J. S., Ott, J., Roy, N., Schneider, N., Smith, R. J., Longmore, S. N., Linz, H.
Publikováno v:
A&A 657, A1 (2022)
The atomic phase of the interstellar medium plays a key role in the formation process of molecular clouds. Due to the line-of-sight confusion in the Galactic plane that is associated with its ubiquity, atomic hydrogen emission has been challenging to
Externí odkaz:
http://arxiv.org/abs/2111.01057