Zobrazeno 1 - 10
of 13 562
pro vyhledávání: '"M49"'
Autor:
AHMAD, Nor Azlina1, ZULKIFLI, Razauden Mohamed1,2 razauden@fbb.utm, HUSSIN, Huszalina1, AMRAN, Syazwani Itri1, NADRI, Muhammad Helmi3, ABDUL RAZAK, Saiful Izwan4, ADAM, Sabrinah5, MOHD YUSOF, Farahwahida2
Publikováno v:
Journal of Research in Pharmacy. 2023, Vol. 27 Issue 1, p232-240. 9p.
Autor:
Wu, Yiming, Liu, Chengze, Peng, Eric W., Ko, Youkyung, Côté, Patrick, Jain, Rashi, Ferrarese, Laura, Yang, Xiaohu, Lançon, Ariane, Puzia, Thomas, Lim, Sungsoon
Combining data from the ACS Virgo Cluster Survey (ACSVCS) and the Next Generation Virgo cluster Survey (NGVS), we extend previous studies of color gradients of the globular cluster (GC) systems of the two most massive galaxies in the Virgo cluster, M
Externí odkaz:
http://arxiv.org/abs/2112.12334
Autor:
Su, Y., Kraft, R. P., Nulsen, P. E. J., Jones, C., Maccarone, T. J., Mernier, F., Lovisari, L., Sheardown, A., Randall, S. W., Roediger, E., Fish, T. M., Forman, W. R., Churazov, E.
The M49 group, resident outside the virial radius of the Virgo cluster, is falling onto the cluster from the south. We report results from deep {\sl XMM-Newton} mosaic observations of M49. Its hot gas temperature is 0.8\,keV at the group center and r
Externí odkaz:
http://arxiv.org/abs/1904.11899
Autor:
Hartke, J., Arnaboldi, M., Gerhard, O., Agnello, A., Longobardi, A., Coccato, L., Pulsoni, C., Freeman, K. C., Merrifield, M.
Publikováno v:
A&A 616, A123 (2018)
M49 (NGC 4472) is the dominant galaxy in subcluster B of the Virgo Cluster, and a benchmark for studying the build-up of the extended halos of brightest group galaxies in the outskirts of galaxy clusters. We investigate the kinematics in the outer ha
Externí odkaz:
http://arxiv.org/abs/1805.03092
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Hartke, J., Arnaboldi, M., Longobardi, A., Gerhard, O., Freeman, K. C., Okamura, S., Nakata, F.
Publikováno v:
A&A 603, A104 (2017)
The galaxy M49 (NGC 4472) is the brightest early-type galaxy in the Virgo Cluster. It is located in Subcluster B and has an unusually blue, metal-poor outer halo. Planetary nebulae (PNe) are excellent tracers of diffuse galaxy and intragroup light. W
Externí odkaz:
http://arxiv.org/abs/1703.06146
Autor:
Liu, Chengze, Peng, Eric W., Cote, Patrick, Ferrarese, Laura, Jordan, Andres, Mihos, J. Christopher, Zhang, Hong-Xin, Munoz, Roberto P., Puzia, Thomas H., Lancon, Ariane, Gwyn, Stephen, Cuillandre, Jean-Charles, Blakeslee, John P., Boselli, Alessandro, Durrell, Patrick R., Duc, Pierre-Alain, Guhathakurta, Puragra, MacArthur, Lauren A., Mei, Simona, Sanchez-Janssen, Ruben, Xu, Haiguang
We use imaging from the Next Generation Virgo cluster Survey (NGVS) to present a comparative study of ultra-compact dwarf (UCD) galaxies associated with three prominent Virgo sub-clusters: those centered on the massive, red-sequence galaxies M87, M49
Externí odkaz:
http://arxiv.org/abs/1508.07334
Publikováno v:
In Drug and Alcohol Dependence 1 July 2024 260 Supplement
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
We use deep surface photometry of the giant elliptical M49 (NGC 4472), obtained as part of our survey for diffuse light in the Virgo Cluster, to study the stellar populations in its outer halo. Our data trace M49's stellar halo out to ~ 100 kpc (7 Re
Externí odkaz:
http://arxiv.org/abs/1301.4898