Zobrazeno 1 - 10
of 209
pro vyhledávání: '"Loubser, S."'
Autor:
Zewdie, Dejene, Assef, Roberto J., Lambert, Trystan, Mazzucchelli, Chiara, Loubser, S. Ilani, Aravena, Manuel, González-López, Jorge, Jun, Hyunsung D., Tsai, Chao-Wei, Stern, Daniel, Li, Guodong, Aranda, Román Fernández, Díaz-Santos, Tanio, Eisenhardt, Peter R. M., Vayner, Andrey, Martin, Lee R., Blain, Andrew W., Wu, Jingwen
Hot dust-obscured galaxies (Hot DOGs), are a family of hyper-luminous, heavily obscured quasars. A number of studies have shown that these objects reside in significantly overdense regions of the Universe based on the identification of companions at
Externí odkaz:
http://arxiv.org/abs/2412.04436
Autor:
Zabel, Nikki, Loni, Alessandro, Sarzi, Marc, Serra, Paolo, Chawla, Arjun, Davis, Timothy A., Kleiner, Dane, Loubser, S. Ilani, Peletier, Reynier
We combine new and archival MUSE observations with data from the MeerKAT Fornax Survey and the ALMA Fornax Cluster Survey to study the ionised, atomic, and molecular gas in six gas-rich dwarf galaxies in the Fornax cluster in detail. We compare the d
Externí odkaz:
http://arxiv.org/abs/2411.02931
Autor:
Rajpurohit, K., O'Sullivan, E., Schellenberger, G., Brienza, M., Vrtilek, J. M., Forman, W., David, L. P., Clarke, T., Botteon, A., Vazza, F., Giacintucci, S., Jones, C., Brüggen, M., Shimwell, T. W., Drabent, A., Loi, F., Loubser, S. I., Kolokythas, K., Babyk, I., Röttgering, H. J. A.
We present deep, wideband multifrequency radio observations (144 MHz$-$8 GHz) of the remarkable galaxy group NGC 741, which yield crucial insights into the interaction between the infalling head-tail radio galaxy (NGC 742) and the main group. Our new
Externí odkaz:
http://arxiv.org/abs/2408.15197
Autor:
Serra, P., Oosterloo, T. A., Kamphuis, P., Jozsa, G. I. G., de Blok, W. J. G., Bryan, G. L., van Gorkom, J. H., Iodice, E., Kleiner, D., Loni, A., Loubser, S. I., Maccagni, F. M., Molnar, D., Peletier, R., Pisano, D. J., Ramatsoku, M., Smith, M. W. L., Verheijen, M. A. W., Zabel, N.
Publikováno v:
A&A 690, A4 (2024)
We present MeerKAT Fornax Survey HI observations of NGC 1427A, a blue irregular galaxy with a stellar mass of 2e+9 Msun located near the centre of the Fornax galaxy cluster. Thanks to the excellent resolution (1 to 6 kpc spatially, 1.4 km/s in veloci
Externí odkaz:
http://arxiv.org/abs/2407.09082
Autor:
Hough, Renier T., Shao, Zhiwei, Cui, Weiguang, Loubser, S. Ilani, Babul, Arif, Davé, Romeel, Rennehan, Douglas, Kobayashi, Chiaki
The newly updated \texttt{GIZMO} and \texttt{Simba} based simulation, \texttt{Simba-C}, with its new stellar feedback, chemical enrichment, and recalibrated AGN feedback, allows for a detailed study of the intragroup medium X-ray properties. We discu
Externí odkaz:
http://arxiv.org/abs/2406.04761
Autor:
de Blok, W. J. G., Healy, J., Maccagni, F. M., Pisano, D. J., Bosma, A., English, J., Jarrett, T., Marasco, A., Meurer, G. R., Veronese, S., Bigiel, F., Chemin, L., Fraternali, F., Holwerda, B. W., Kamphuis, P., Klöckner, H. R., Kleiner, D., Leroy, A. K., Mogotsi, M., Oman, K. A., Schinnerer, E., Verdes-Montenegro, L., Westmeier, T., Wong, O. I., Zabel, N., Amram, P., Carignan, C., Combes, F., Brinks, E., Dettmar, R. J., Gibson, B. K., Jozsa, G. I. G., Koribalski, B. S., McGaugh, S. S., Oosterloo, T. A., Spekkens, K., Schröder, A. C., Adams, E. A. K., Athanassoula, E., Bershady, M. A., Beswick, R. J., Blyth, S., Elson, E. C., Frank, B. S., Heald, G., Henning, P. A., Kurapati, S., Loubser, S. I., Lucero, D., Meyer, M., Namumba, B., Oh, S. -H., Sardone, A., Sheth, K., Smith, M. W. L., Sorgho, A., Walter, F., Williams, T., Woudt, P. A., Zijlstra, A.
Publikováno v:
A&A 688, A109 (2024)
The MHONGOOSE (MeerKAT HI Observations of Nearby Galactic Objects: Observing Southern Emitters) survey maps the distribution and kinematics of the neutral atomic hydrogen (HI) gas in and around 30 nearby star-forming spiral and dwarf galaxies to extr
Externí odkaz:
http://arxiv.org/abs/2404.01774
Autor:
Hough, Renier T., Rennehan, Douglas, Kobayashi, Chiaki, Loubser, S. Ilani, Davé, Romeel, Babul, Arif, Cui, Weiguang
We introduce a new chemical enrichment and stellar feedback model into GIZMO, using the SIMBA sub-grid models as a base. Based on the state-of-the-art chemical evolution model of Kobayashi et al., SIMBA-C tracks 34 elements from H$\rightarrow$Ge and
Externí odkaz:
http://arxiv.org/abs/2308.03436
Autor:
Kleiner, D., Serra, P., Maccagni, F. M., Raj, M. A., de Blok, W. J. G., Józsa, G. I. G., Kamphuis, P., Kraan-Korteweg, R., Loi, F., Loni, A., Loubser, S. I., Molnár, D. Cs., Oosterloo, T. A., Peletier, R., Pisano, D. J.
Publikováno v:
A&A 675, A108 (2023)
We present MeerKAT Fornax Survey atomic hydrogen (HI) observations of the dwarf galaxies located in the central ~2.5 x 4 deg$^2$ of the Fornax galaxy cluster. The HI images presented in this work have a $3\sigma$ column density sensitivity between 2.
Externí odkaz:
http://arxiv.org/abs/2305.13163
Autor:
Loni, Alessandro, Serra, Paolo, Sarzi, Marc, Józsa, Gyula I. G., Anta, Pablo M. Galán-de, Zabel, Nikki, Kleiner, Dane, Maccagni, Filippo M., Molnár, Daniel, Ramatsoku, Mpati, Loi, Francesca, Corsini, Enrico M., Pisano, D. J., Kamphuis, Peter, Davis, Timothy A., de Blok, W. J. G., Dettmar, Ralf J., Falcon-Barroso, Jesus, Iodice, Enrichetta, Lara-López, Maritza A., Loubser, S. Ilani, Morokuma-Matsui, Kana, Peletier, Reynier, Pinna, Francesca, Poci, Adriano, Smith, Matthew W. L., Trager, Scott C., van de Ven, Glenn
We study the evolutionary path of the Fornax cluster galaxy NGC$~$1436, which is known to be currently transitioning from a spiral into a lenticular morphology. This galaxy hosts an inner star-forming disc and an outer quiescent disc, and we analyse
Externí odkaz:
http://arxiv.org/abs/2305.05709
Autor:
Saeedzadeh, Vida, Jung, S. Lyla, Rennehan, Douglas, Babul, Arif, Tremmel, Michael, Quinn, Thomas R., Shao, Zhiwei, Sharma, Prateek, Mayer, Lucio, OSullivan, E., Loubser, S. Ilani
Using high-resolution {\sc Romulus} simulations, we explore the origin and evolution of the circumgalactic medium (CGM) in the region 0.1 $\leq \mathrm{R}/\mathrm{R}_\mathrm{500} \leq$ 1 around massive central galaxies in group-scale halos. We find t
Externí odkaz:
http://arxiv.org/abs/2304.03798