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

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

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.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-002E-14A2-9 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-002E-14A3-7

Genre: Journal Article

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Creators:
Feng, J.¹, Author
Wu, Q.¹, Author
Lu, R.¹, Author

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1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652

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Free keywords: accretion, accretion disks, black hole physics, galaxies: individual: M87, galaxies: jets

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Dates: Date issued: 2016-10

Publication Status: Issued

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Identifiers: DOI: 10.3847/0004-637X/830/1/6
BibTex Citekey: 2016apj...830....6f

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Title: Astrophysical Journal

Source Genre: Journal

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Pages: - Volume / Issue: 830 Sequence Number: 6 Start / End Page: 6 Identifier: -