(PDF) Investigating the Nature of the $\Mathsf {\Vec

Investigating the Nature of the $\Mathsf {\Vec Z}\simeq\mathsf {2.8}$ Submillimeter Selected Galaxy SMM J02399-0136 With VLT Spectropolarimetry

Astronomy and Astrophysics - France

doi 10.1051/0004-6361:20011442

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Date

December 1, 2001

Authors

J. Vernet

A. Cimatti

Publisher

EDP Sciences

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Amanote Research

Investigating the Nature of the $\Mathsf {\Vec Z}\simeq\mathsf {2.8}$ Submillimeter Selected Galaxy SMM J02399-0136 With VLT Spectropolarimetry

Astronomy and Astrophysics - France

doi 10.1051/0004-6361:20011442

Full Text

Abstract

Categories

Date

Authors

Publisher

Related search

Discovery of a Lyα-Emitting Dark Cloud Within the Z ∼ 2.8 SMM J02399-0136 System

Contribution of Starburst Mergers at ${\Vec Z}\sim\,{\mathsf{1}}$ to the Strong Evolution of Infrared and Submillimeter Deep Surveys

The H$\mathsf{\alpha}$ Galaxy Survey

Two Emission Line Objects With ${\Vec Z}>\mathsf{0.2}$ in the Optical Filament Apparently Connecting the Seyfert Galaxy NGC 7603 to Its Companion

The Warm-Hot Intergalactic Medium at $\Mathsf{\vec {Z}\sim2.2}$: Metal Enrichment and Ionization Source

Extinction and Metal Column Density of HI Regions Up to Redshift Z $\Mathsf{\simeq 2}$

Photometric Study of the Double Cluster $\Vec H$ & $\Mathsf{\chi}$ Persei

High-Excitation CO in a Quasar Host Galaxy at Z $\Mathsf{=6.42}$

Elementary Reactions of the Phenyl Radical, C$_\mathsf{6}$H$_\mathsf{5}$, With C$_\mathsf{3}$H$_\mathsf{4}$ Isomers, and of Benzene, C$_\mathsf{6}$H$_\mathsf{6}$, With Atomic Carbon in Extraterrestrial Environments