Star formation in M 33: multiwavelength signatures across the disk
2008; EDP Sciences; Volume: 493; Issue: 2 Linguagem: Inglês
10.1051/0004-6361
ISSN1432-0746
AutoresS. Verley, E. Corbelli, C. Giovanardi, L. K. Hunt,
Tópico(s)Astrophysical Phenomena and Observations
ResumoAims. We use different tracers, such as Hα, ultraviolet (UV), and infrared (IR) emissions at various wavelengths, to study the dust and star formation (SF) conditions throughout the disk of M 33.
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