scholarly journals The ACS Virgo Cluster Survey. VII. Resolving the Connection between Globular Clusters and Ultracompact Dwarf Galaxies

2005 ◽  
Vol 627 (1) ◽  
pp. 203-223 ◽  
Author(s):  
Monica Haşegan ◽  
Andres Jordan ◽  
Patrick Cote ◽  
S. G. Djorgovski ◽  
Dean E. McLaughlin ◽  
...  
2018 ◽  
Vol 14 (S344) ◽  
pp. 384-388
Author(s):  
Chengze Liu ◽  
Eric W. Peng ◽  
Patrick Côté ◽  
Hong-Xin Zhang ◽  
Laura Ferrarese ◽  
...  

AbstractBased on the data from the Next Generation Virgo cluster Survey (NGVS), we statistically study the photometric properties of globular clusters (GCs), ultra-compact dwarfs (UCDs) and dwarf nuclei in the Virgo core (M87) region. We found an obvious negative color (g - z) gradient in GC system associate with M87, i.e. GCs in the outer regions are bluer. However, such color gradient does not exist in UCD system, neither in dwarf nuclei system around M87. In addition, we found that many UCDs are surrounded by extended, low surface brightness envelopes. The dwarf nuclei and UCDs show different spatial distributions from GCs, with dwarf nuclei and UCDs (especially for the UCDs with visible envelopes) lying at larger distances to the Virgo center. These results support the view that UCDs (at least for a fraction of UCDs) are more tied to dwarf nuclei than to GCs.


2008 ◽  
Vol 681 (1) ◽  
pp. 197-224 ◽  
Author(s):  
Eric W. Peng ◽  
Andrés Jordán ◽  
Patrick Côté ◽  
Marianne Takamiya ◽  
Michael J. West ◽  
...  

2015 ◽  
Vol 11 (S317) ◽  
pp. 153-158
Author(s):  
Eric W. Peng ◽  
Hong-Xin Zhang ◽  
Chengze Liu ◽  
Yiqing Liu

AbstractAt the center of the nearest galaxy cluster, the Virgo cluster, lies the massive cD galaxy, M87 (NGC 4486). Using data from the Next Generation Virgo Cluster Survey, we investigate the relationship between M87, its globular clusters (GCs), and satellite dwarf galaxies. We find that the kinematics of GCs and ultra-compact dwarfs (UCDs) are different, indicating that UCDs are not simply massive GCs. We also identify a morphological sequence of envelope fraction around UCDs correlated with cluster-centric distance that suggest UCDs are the result of tidal stripping. Lastly, we find that the [α/Fe] abundance ratios of low-mass early-type galaxies in Virgo exhibit a strong negative gradient within ~ 400 kpc of M87, where the galaxies closest to M87 have the highest values. These satellite galaxies are likely the surviving counterparts of accreted dwarfs that contribute stars to the metal-poor, α-rich stellar halos of massive galaxies. Together, these results describe a dense environment that has had a strong and continuing impact on the evolution of its low-mass neighbors.


2017 ◽  
Vol 844 (2) ◽  
pp. 104 ◽  
Author(s):  
Mathieu Powalka ◽  
Ariane Lançon ◽  
Thomas H. Puzia ◽  
Eric W. Peng ◽  
Chengze Liu ◽  
...  

2018 ◽  
Vol 864 (1) ◽  
pp. 36 ◽  
Author(s):  
Alessia Longobardi ◽  
Eric W. Peng ◽  
Patrick Côté ◽  
J. Christopher Mihos ◽  
Laura Ferrarese ◽  
...  

2011 ◽  
Vol 48 ◽  
pp. 345-350
Author(s):  
P.-A. Duc ◽  
L. Ferrarese ◽  
J.-C. Cuillandre ◽  
S. Gwyn ◽  
L.A. MacArthur ◽  
...  

2004 ◽  
Vol 613 (1) ◽  
pp. 279-301 ◽  
Author(s):  
Andres Jordan ◽  
Patrick Cote ◽  
Laura Ferrarese ◽  
John P. Blakeslee ◽  
Simona Mei ◽  
...  

2019 ◽  
Vol 885 (2) ◽  
pp. 145
Author(s):  
Weijia Sun ◽  
Eric W. Peng ◽  
Youkyung Ko ◽  
Patrick Côté ◽  
Laura Ferrarese ◽  
...  

2013 ◽  
Vol 436 (2) ◽  
pp. 1057-1073 ◽  
Author(s):  
Ilse De Looze ◽  
Maarten Baes ◽  
Alessandro Boselli ◽  
Luca Cortese ◽  
Jacopo Fritz ◽  
...  

2015 ◽  
Vol 802 (1) ◽  
pp. 30 ◽  
Author(s):  
Hong-Xin Zhang ◽  
Eric W. Peng ◽  
Patrick Côté ◽  
Chengze Liu ◽  
Laura Ferrarese ◽  
...  

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