Modeling Star Formation in Dwarf Spheroidal Galaxies: A Case for Extended Dark Matter Halos

2005 ◽  
Vol 624 (2) ◽  
pp. 726-741 ◽  
Author(s):  
Sergey Mashchenko ◽  
H. M. P. Couchman ◽  
Alison Sills
2010 ◽  
Vol 717 (2) ◽  
pp. L87-L91 ◽  
Author(s):  
Matthew G. Walker ◽  
Stacy S. McGaugh ◽  
Mario Mateo ◽  
Edward W. Olszewski ◽  
Rachel Kuzio de Naray

1998 ◽  
Vol 11 (1) ◽  
pp. 121-122
Author(s):  
Claude Carignan

Recent studies (Puche & Westpfahl 1994, Young & Lo 1996) have shown that the distribution of HI in some extreme low luminosity dwarf irregular galaxies (e.g. M81dwA, Holmberg I, Leo A) tends to have a ring-like (or shell-like) distribution which suggests that a single burst of star formation could expell most of the remaining ISM (or at least a large fraction of it) from the system. In view of this, Puche & Westpfahl (1994) suggested that in dwarf spheroidal galaxies, the HI should be found at large radii since no young stellar population is observed in most of them.


2018 ◽  
Vol 98 (4) ◽  
Author(s):  
Sebastian Bergström ◽  
Riccardo Catena ◽  
Andrea Chiappo ◽  
Jan Conrad ◽  
Björn Eurenius ◽  
...  

2017 ◽  
Vol 468 (2) ◽  
pp. 1338-1348 ◽  
Author(s):  
Shu-Rong Chen ◽  
Hsi-Yu Schive ◽  
Tzihong Chiueh

2013 ◽  
Vol 557 ◽  
pp. A66 ◽  
Author(s):  
Matthieu Béthermin ◽  
Lingyu Wang ◽  
Olivier Doré ◽  
Guilaine Lagache ◽  
Mark Sargent ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document