Zobrazeno 1 - 10
of 1 817
pro vyhledávání: '"Johnston E."'
Autor:
Lopez, S., Afruni, A., Zamora, D., Tejos, N., Ledoux, C., Hernandez, J., Berg, T. A. M., Cortes, H., Urbina, F., Johnston, E. J., Barrientos, L. F., Bayliss, M. B., Cuellar, R., Krogager, J. K., Noterdaeme, P., Solimano, M.
We present VLT/MUSE integral-field spectroscopy ($R\approx 1\,800$) of four giant gravitational arcs exhibiting strong C IV absorption at 8 intervening redshifts, $z_{abs}\approx 2.0$--$2.5$. We detect C IV absorption in a total of 222 adjacent and s
Externí odkaz:
http://arxiv.org/abs/2410.03029
Autor:
Kreckel, K., Egorov, O. V., Egorova, E., Blanc, G. A., Drory, N., Kounkel, M., Mendez-Delgado, J. E., Roman-Zuniga, C. G., Sanchez, S. F., Stringfellow, G. S., Stutz, A. M., Zari, E., Barrera-Ballesteros, J. K., Bizyaev, D., Brownstein, J. R., Congiu, E., Fernandez-Trincado, J. G., Garcia, P., Hillenbrand, L., Ibarra-Medel, H. J., Jin, Y., Johnston, E. J., Jones, A. M., Kim, J. Serena, Kollmeier, J. A., Kong, S., Krishnarao, D., Kumari, N., Li, J., Long, K., Mata-Sanchez, A., Mejia-Narvaez, A., Popa, S. A., Rix, H-W, Sattler, N., Serna, J., Singh, A., Sanchez-Gallego, J. R., Wofford, A., Wong, T.
Publikováno v:
A&A 689, A352 (2024)
The Orion Molecular Cloud complex, one of the nearest (D = 406 pc) and most extensively studied massive star-forming regions, is ideal for constraining the physics of stellar feedback, but its ~12 deg diameter on the sky requires a dedicated approach
Externí odkaz:
http://arxiv.org/abs/2405.14943
Autor:
Solimano, M., González-López, J., Aravena, M., Herrera-Camus, R., De Looze, I., Schreiber, N. M. Förster, Spilker, J., Tadaki, K., Assef, R. J., Barcos-Muñoz, L., Davies, R. L., Díaz-Santos, T., Ferrara, A., Fisher, D. B., Guaita, L., Ikeda, R., Johnston, E. J., Lutz, D., Mitsuhashi, I., Moya-Sierralta, C., Relaño, M., Naab, T., Posses, A. C., Telikova, K., Übler, H., van der Giessen, S., Villanueva, V.
Publikováno v:
A&A 689, A145 (2024)
Massive star-forming galaxies in the high-redshift universe host large reservoirs of cold gas in their circumgalactic medium (CGM). Traditionally, these reservoirs have been linked to diffuse H I Lyman-$\alpha$ (Ly$\alpha)$ emission extending beyond
Externí odkaz:
http://arxiv.org/abs/2401.04919
Autor:
Afruni, A., Lopez, S., Anshul, P., Tejos, N., Noterdaeme, P., Berg, T. A. M., Ledoux, C., Solimano, M., Gonzalez-Lopez, J., Gronke, M., Barrientos, F., Johnston, E. J.
Publikováno v:
A&A 680, A112 (2023)
One of the biggest puzzles regarding the circumgalactic medium (CGM) is the structure of its cool ($T\sim10^4$ K) gas phase. While the kinematics of quasar absorption systems suggests the CGM is composed of a population of different clouds, constrain
Externí odkaz:
http://arxiv.org/abs/2310.13732
Autor:
Junais, Weilbacher, P. M., Epinat, B., Boissier, S., Galaz, G., Johnston, E. J., Puzia, T. H., Amram, P., Małek, K.
Publikováno v:
A&A 681, A100 (2024)
Giant low-surface brightness (GLSB) galaxies are an extreme class of objects with very faint and extended gas-rich disks. Malin 1 is the largest GLSB galaxy known to date, but its formation is still poorly understood. We use VLT/MUSE IFU spectroscopi
Externí odkaz:
http://arxiv.org/abs/2310.11872