Properties of Low Surface Brightness Galaxies and Normal Spirals in the Near-Infrared

2002 ◽  
Vol 124 (3) ◽  
pp. 1360-1379 ◽  
Author(s):  
Gaspar Galaz ◽  
Julianne J. Dalcanton ◽  
Leopoldo Infante ◽  
Ezequiel Treister
2003 ◽  
Vol 405 (1) ◽  
pp. 99-109 ◽  
Author(s):  
D. Monnier Ragaigne ◽  
W. van Driel ◽  
S. E. Schneider ◽  
T. H. Jarrett ◽  
C. Balkowski

2003 ◽  
Vol 408 (1) ◽  
pp. 67-78 ◽  
Author(s):  
D. Monnier Ragaigne ◽  
W. van Driel ◽  
K. O'Neil ◽  
S. E. Schneider ◽  
C. Balkowski ◽  
...  

1999 ◽  
Vol 171 ◽  
pp. 245-252
Author(s):  
E.F. Bell ◽  
R.G. Bower ◽  
R.S. de Jong ◽  
B.J. Rauscher ◽  
D. Barnaby ◽  
...  

AbstractNear-infrared images of a sample of red, blue and giant low surface brightness disk galaxies (LSBGs) were combined with optical data with the aim of constraining their star formation histories. Most LSBGs have strong colour gradients consistent with mean stellar age gradients. We find that LSBGs have a large range of ages and metallicities, spanning those observed in normal disk galaxies. In particular, red and blue LSBGs have very different star formation histories and represent two independent routes to low B band surface brightness. Blue LSBGs are well described by models with low, roughly constant star formation rates, whereas red LSBGs are better described by a ‘faded disk’ scenario.


2003 ◽  
Vol 408 (2) ◽  
pp. 465-477 ◽  
Author(s):  
D. Monnier Ragaigne ◽  
W. van Driel ◽  
S. E. Schneider ◽  
C. Balkowski ◽  
T. H. Jarrett

1999 ◽  
Vol 118 (3) ◽  
pp. 1220-1229 ◽  
Author(s):  
Taft E. Armandroff ◽  
George H. Jacoby ◽  
James E. Davies

1999 ◽  
Vol 514 (2) ◽  
pp. L83-L86 ◽  
Author(s):  
Raul Jimenez ◽  
David V. Bowen ◽  
Francesca Matteucci

2006 ◽  
Vol 459 (3) ◽  
pp. 679-692 ◽  
Author(s):  
C. Adami ◽  
R. Scheidegger ◽  
M. Ulmer ◽  
F. Durret ◽  
A. Mazure ◽  
...  

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