An Accretion-jet Model for M87: Interpreting the Spectral Energy Distribution 
and Faraday Rotation Measure

Feng, J.; Wu, Q.; Lu, R.

doi:10.3847/0004-637X/830/1/6

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

An Accretion-jet Model for M87: Interpreting the Spectral Energy Distribution and Faraday Rotation Measure

MPS-Authors

Feng, J.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Wu, Q.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Lu, R.
Max Planck Institute for Radio Astronomy, 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

Feng, J., Wu, Q., & Lu, R. (2016). An Accretion-jet Model for M87: Interpreting the Spectral Energy Distribution and Faraday Rotation Measure. Astrophysical Journal, 830: 6, pp. 6. doi:10.3847/0004-637X/830/1/6.

Cite as: https://hdl.handle.net/11858/00-001M-0000-002E-14A2-9

Abstract

There is no abstract available