Zobrazeno 1 - 10
of 193
pro vyhledávání: '"Stil, J"'
Autor:
Raycheva, N., Haverkorn, M., Ideguchi, S., Stil, J. M., Sun, X., Han, J. L., Carretti, E., Gao, X. Y., Bracco, A., Clark, S. E., Dickey, J. M., Gaensler, B. M., Hill, A., Landecker, T., Ordog, A., Seta, A., Tahani, M., Wolleben, M.
Faraday tomography of broadband radio polarization surveys enables us to study magnetic fields and their interaction with the interstellar medium (ISM). Such surveys include the Global Magneto-Ionic Medium Survey (GMIMS), which covers the northern an
Externí odkaz:
http://arxiv.org/abs/2406.06166
Autor:
Taylor, A. R., Sekhar, S., Heino, L., Scaife, A. M. M., Stil, J., Bowles, M., Jarvis, M., Heywood, I., Collier, J. D.
The MeerKAT International GigaHertz Tiered Extragalactic Exploration (MIGHTEE) is one of the MeerKAT large survey projects, designed to pathfind SKA key science. MIGHTEE is undertaking deep radio imaging of four well observed fields (COSMOS, XMM-LSS,
Externí odkaz:
http://arxiv.org/abs/2312.13230
Autor:
Syed, J., Beuther, H., Goldsmith, P. F., Henning, Th., Heyer, M., Klessen, R. S., Stil, J. M., Soler, J. D., Anderson, L. D., Urquhart, J. S., Rugel, M. R., Johnston, K. G., Brunthaler, A.
Stars form in the dense interiors of molecular clouds. The dynamics and physical properties of the atomic interstellar medium (ISM) set the conditions under which molecular clouds and eventually stars will form. It is, therefore, critical to investig
Externí odkaz:
http://arxiv.org/abs/2310.02077
Autor:
Böckmann, K., Brüggen, M., Heesen, V., Basu, A., O'Sullivan, S. P., Heywood, I., Jarvis, M., Scaife, A., Stil, J., Taylor, R., Adams, N. J., Bowler, R. A. A., Tudorache, M. N.
Publikováno v:
A&A 678, A56 (2023)
The detection and study of magnetic fields surrounding galaxies is important to understand galaxy evolution since magnetic fields are tracers for dynamical processes in the circumgalactic medium (CGM) and can have a significant impact on the evolutio
Externí odkaz:
http://arxiv.org/abs/2308.11391
Publikováno v:
2023
We measure the specific star formation rates of \textit{K}-band selected galaxies from the ELAIS-N1 by stacking GMRT data at 610 MHz. We identify a sample of SFGs, spanning $\rm{0.1\leq\,\textit{z}\,\leq\,1.5}$ and $\rm{10^{8.5}<\,{\textit{M}_{\star}
Externí odkaz:
http://arxiv.org/abs/2307.04152
Autor:
West, J. L., Campbell, J. L., Bhaura, P., Kothes, R., Safi-Harb, S., Stil, J. M., Taylor, A. R., Foster, T., Gaensler, B. M., George, S. J., Gibson, S. J., Ricci, R.
Using data from the Galactic Arecibo L-band Feed Array Continuum Transit Survey (GALFACTS), we report the discovery of two previously unidentified, very compressed, thin, and straight polarized filaments approximately centred at Galactic coordinates,
Externí odkaz:
http://arxiv.org/abs/2210.10098
Autor:
Raycheva, N. C., Haverkorn, M., Ideguchi, S., Stil, J. M., Gaensler, B. M., Sun, X., Han, J. L., Carretti, E., Gao, X. Y., Wijte, T.
Publikováno v:
A&A 663, A170 (2022)
Magnetic fields in the turbulent interstellar medium (ISM) are a key element in understanding Galactic dynamics, but there are many observational challenges. One useful probe for studying the magnetic field component parallel to the line of sight (Lo
Externí odkaz:
http://arxiv.org/abs/2206.01787
Autor:
Campbell, J. L., Clark, S. E., Gaensler, B. M., Marchal, A., Van Eck, C. L., Deshpande, A. A., George, S. J., Gibson, S. J., Ricci, R., Stil, J. M., Taylor, A. R.
Understanding how the Galactic magnetic field threads the multi-phase interstellar medium (ISM) remains a considerable challenge, as different magnetic field tracers probe dissimilar phases and field components. We search for evidence of a common mag
Externí odkaz:
http://arxiv.org/abs/2112.03247
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
Publikováno v:
Universe 2021, 7(9), 338
Young Supernova remnants (SNRs) with smaller angular sizes are likely missing from existing radio SNR catalogues, caused by observational constraints and selection effects. In order to find new compact radio SNR candidates, we searched the high angul
Externí odkaz:
http://arxiv.org/abs/2109.07003