TY  - GEN 
AU  - Lisenfeld , Ute
AU  - Ferrara, A.
PY  - 1998
SN  - 0004-637X
SN  - 1538-4357
UR  - http://hdl.handle.net/10481/29061
AB  - We have compared the metallicity (represented by oxygen abundance), and the dust-to-gas ratio, in a sample of dwarf galaxies. For dwarf irregulars (dIrrs) we find a good correlation between the two quantities, with a power-law index 0.54±0.2. Blue...
LA  - eng
PB  - American Astronomical Society; Institute of Physics (IOP)
KW  - ISM
KW  - Abundances
KW  - Dust
KW  - Extinction
KW  - Galaxies
KW  - Irregulars
KW  - Evolution
KW  - Infrared
TI  - Dust-to-gas ratio and metal abundance in dwarf galaxies
ER  -