Zobrazeno 1 - 10
of 466
pro vyhledávání: '"JACKSON, J. M."'
Autor:
Heidari, N., H'ebrard, G., Martioli, E., Eastman, J. D., Jackson, J. M., Delfosse, X., Jord'an, A., Correia, A. C. M., Sousa, S., Dragomir, D., Forveille, T., Boisse, I., Giacalone, S. A., D'iaz, R. F., Brahm, R., Almasian, D., Almenara, J. M., Bieryla, A., Barkaoui, K., Baker, D., Barros, S. C. C ., Bonfils, X., Carmona, A., Collins, K. A., Cort'es-Zuleta, P., Deleuil, M., Demangeon, O. D. S., Edwards, B., Eberhardt, J., Espinoza, N., Eisner, N., Feliz, D. L., Frommer, A. C., Fukui, A., Grau, F., Gupta, A. F., Hara, N., Hobson, M. J., Henning, T., Howell, S. B., Jenkins, J. M., Kiefer, F., LaCourse, D. M., Laskar, J., Law, N., Mann, A. W., Murgas, F., Moutou, C., Narita, N., Palle, E., Relles, H. M., Stassun, K. G., Bell, J. Serrano, Schwarz, R. P., Srdoc, G., Strøm, P. A., Safonov, B., Sarkis, P., Schlecker, M., Pinto, M. Tala, Pepper, J., Rojas, F. I., Twicken, J. D., Trifonov, T., Villanueva Jr, S., Watkins, C. N., Winn, J. N., Ziegler, C.
We present the study of seven systems, three of which TOI-2295, TOI-2537, and TOI-5110 are newly discovered planetary systems. Through the analysis of TESS photometry, SOPHIE radial velocities, and high-spatial resolution imaging, we found that TOI-2
Externí odkaz:
http://arxiv.org/abs/2412.08527
Autor:
Polles, F. L., Fadda, D., Vacca, W. D., Abel, N. P., Chevance, M., Fischer, C., Jackson, J. M., Lebouteiller, V., Madden, S., Ramambason, L.
We present the [OIII]52{\mu}m map of the dwarf galaxy IC10, obtained with the Field-Imaging Far-Infrared Line Spectrometer (FIFI-LS) on board the Stratospheric Observatory for Infrared Astronomy (SOFIA). We combine the [OIII]52{\mu}m map with Hersche
Externí odkaz:
http://arxiv.org/abs/2407.04790
Autor:
Jackson, J. M., Whitaker, J. S., Chambers, E. T., Simon, R., Guevara, C., Allingham, D., Patterson, P., Killerby-Smith, N., Askew, J., Vandenberg, T., Smith, H. A., Sanhueza, P., Stephens, I. W., Bonne, L., Polles, F., Schmiedeke, A., Honigh, N., Justen, M.
Using the upGREAT instrument on SOFIA, we have imaged [C II] 157.74 and [O I] 63.18 micron line emission from a bright photodissociation region (PDR) associated with an ionized ``bubble'' located in the Nessie Nebula, a filamentary infrared dark clou
Externí odkaz:
http://arxiv.org/abs/2402.11062
Autor:
Wang, Chao, Wang, Ke, Xu, Feng-Wei, Sanhueza, Patricio, Liu, Hauyu Baobab, Zhang, Qizhou, Lu, Xing, Fontani, F., Caselli, Paola, Busquet, Gemma, Tan, Jonathan C., Li, Di, Jackson, J. M., Pillai, Thushara, Ho, Paul T. P., Guzmán, Andrés E., Yue, Nannan
Context. Traditionally, supersonic turbulence is considered to be one of the most likely mechanisms to slow down the gravitational collapse in dense clumps, thereby enabling the formation of massive stars. However, several recent studies have raised
Externí odkaz:
http://arxiv.org/abs/2310.17970
Autor:
Bonne, L., Bontemps, S., Schneider, N., Simon, R., Clarke, S. D., Csengeri, T., Chambers, E., Graf, U., Jackson, J. M., Klein, R., Okada, Y., Tielens, A. G. G. M., Tiwari, M.
We present new $^{13}$CO(1-0), C$^{18}$O(1-0), HCO$^{+}$(1-0) and H$^{13}$CO$^{+}$(1-0) maps from the IRAM 30m telescope, and a spectrally-resolved [CII] 158 $\mu$m map observed with the SOFIA telescope towards the massive DR21 cloud. This traces the
Externí odkaz:
http://arxiv.org/abs/2305.07785
Autor:
Henshaw, J. D., Ginsburg, A., Haworth, T. J., Longmore, S. N., Kruijssen, J. M. D., Mills, E. A. C., Sokolov, V., Walker, D. L., Barnes, A. T., Contreras, Y., Bally, J., Battersby, C., Beuther, H., Butterfield, N., Dale, J. E., Henning, T., Jackson, J. M., Kauffmann, J., Pillai, T., Ragan, S., Riener, M., Zhang, Q.
In this paper we provide a comprehensive description of the internal dynamics of G0.253+0.016 (a.k.a. 'the Brick'); one of the most massive and dense molecular clouds in the Galaxy to lack signatures of widespread star formation. As a potential host
Externí odkaz:
http://arxiv.org/abs/1902.02793
Autor:
Kruijssen, J. M. D., Dale, J. E., Longmore, S. N., Walker, D. L., Henshaw, J. D., Jeffreson, S. M. R., Petkova, M. A., Ginsburg, A., Barnes, A. T., Battersby, C. D., Immer, K., Jackson, J. M., Keto, E. R., Krieger, N., Mills, E. A. C., Sánchez-Monge, Á., Schmiedeke, A., Suri, S. T., Zhang, Q.
The evolution of molecular clouds in galactic centres is thought to differ from that in galactic discs due to a significant influence of the external gravitational potential. We present a set of numerical simulations of molecular clouds orbiting on t
Externí odkaz:
http://arxiv.org/abs/1902.01860
Autor:
Federrath, C., Rathborne, J. M., Longmore, S. N., Kruijssen, J. M. D., Bally, J., Contreras, Y., Crocker, R. M., Garay, G., Jackson, J. M., Testi, L., Walsh, A. J.
Star formation in the Galactic disc is primarily controlled by gravity, turbulence, and magnetic fields. It is not clear that this also applies to star formation near the Galactic Centre. Here we determine the turbulence and star formation in the CMZ
Externí odkaz:
http://arxiv.org/abs/1609.08726
Autor:
Federrath, C., Rathborne, J. M., Longmore, S. N., Kruijssen, J. M. D., Bally, J., Contreras, Y., Crocker, R. M., Garay, G., Jackson, J. M., Testi, L., Walsh, A. J.
Publikováno v:
C. Federrath et al 2016 ApJ 832 143
Star formation is primarily controlled by the interplay between gravity, turbulence, and magnetic fields. However, the turbulence and magnetic fields in molecular clouds near the Galactic Center may differ substantially from spiral-arm clouds. Here w
Externí odkaz:
http://arxiv.org/abs/1609.05911
Autor:
Deharveng, L., Zavagno, A., Samal, M. R., Anderson, L. D., LeLeu, G., Brevot, D., Duarte-Cabral, A., Molinari, S., Pestalozzi, M., Foster, J. B., Rathborne, J. M., Jackson, J. M.
Publikováno v:
A&A 582, A1 (2015)
Our goal is to identify bipolar HII regions and to understand their morphology, their evolution, and the role they play in the formation of new generations of stars. We use the Spitzer and Herschel Hi-GAL surveys to identify bipolar HII regions. We s
Externí odkaz:
http://arxiv.org/abs/1507.00215