scholarly journals Cold, Old, and Metal-poor: New Stellar Substructures in the Milky Way’s Dwarf Spheroidals

2019 ◽  
Vol 878 (2) ◽  
pp. 152 ◽  
Author(s):  
V. Lora ◽  
E. K. Grebel ◽  
S. Schmeja ◽  
A. Koch
Keyword(s):  
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.


2013 ◽  
Vol 763 (2) ◽  
pp. 91 ◽  
Author(s):  
John R. Jardel ◽  
Karl Gebhardt ◽  
Maximilian H. Fabricius ◽  
Niv Drory ◽  
Michael J. Williams

2011 ◽  
Vol 729 (1) ◽  
pp. 23 ◽  
Author(s):  
Crystal M. Brasseur ◽  
Nicolas F. Martin ◽  
Hans-Walter Rix ◽  
Mike Irwin ◽  
Annette M. N. Ferguson ◽  
...  
Keyword(s):  

2006 ◽  
Vol 367 (1) ◽  
pp. 387-399 ◽  
Author(s):  
J. I. Read ◽  
M. I. Wilkinson ◽  
N. W. Evans ◽  
G. Gilmore ◽  
J. T. Kleyna

2003 ◽  
Vol 397 (3) ◽  
pp. L9-L12 ◽  
Author(s):  
M. Hilker ◽  
S. Mieske ◽  
L. Infante

2009 ◽  
Vol 698 (1) ◽  
pp. 222-232 ◽  
Author(s):  
Jorge Peñarrubia ◽  
Julio F. Navarro ◽  
Alan W. McConnachie ◽  
Nicolas F. Martin

1999 ◽  
Vol 192 ◽  
pp. 455-458 ◽  
Author(s):  
F. Kerschbaum ◽  
W. Nowotny ◽  
J. Hron ◽  
M. Schultheis

This paper is based on photometry from two different observational approaches. Both are of an explorative character and act as feasibility studies. For the future we plan to use these methods to study Asymptotic Giant Branch (AGB) stars in nearby galaxies.First, we present results on broad-band photometry in Bessell V and I, as well as narrow-band measurements in the Wing 778 nm and 812 nm filters of a galactic globular cluster using the new Austrian Oe-FOSC (Oesterreich Faint Object Spectrograph and Camera), a copy of the ESO Instrument EFOSC mounted on our 1.5 m-telescope.The second part of the contribution deals with the possibilities of using Gunn I, J and KS measurements originating from the DENIS (DEep Near Infrared Survey of the Southern Sky) project on similar objects. A few southern dwarf spheroidals already observed within DENIS (covering now some 40% of the southern hemisphere) are selected.


1986 ◽  
Vol 91 ◽  
pp. 1091 ◽  
Author(s):  
N. B. Suntzeff ◽  
M. Aaronson ◽  
E. W. Olszewski ◽  
K. H. Cook
Keyword(s):  

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