Dust emission in the far-infrared as a star formation tracer at z = 0: 
systematic trends with luminosity

Pierini, D.; Möller, C. S.

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

Dust emission in the far-infrared as a star formation tracer at z = 0: systematic trends with luminosity

MPS-Authors

/persons/resource/persons16296

Pierini, D.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

Möller, C. S.
Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Pierini, D., & Möller, C. S. (2003). Dust emission in the far-infrared as a star formation tracer at z = 0: systematic trends with luminosity. Monthly Notices of the Royal Astronomical Society, 346, 818-824.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-E86E-2

Abstract

There is no abstract available