Published August 20, 2010 | Version v1
Journal article

HIGHLY POLARIZED COUNTERPART OF THE DOUBLE HELIX NEBULA

  • 1. Institute of Space and Astronautical Science, Sagamihara, Kanagawa 252-5210 (Japan)
  • 2. Institute of Astronomy, University of Tokyo, Mitaka, Tokyo 181-0015 (Japan)

Description

We identified the double helix nebula (DHN) found by the Spitzer Space Telescopein the Galactic center region as a highly polarized feature at 10 GHz with the Nobeyama 45 m telescope. The DHN is located near the north end of the polarized plumes. The position angles of Faraday rotation corrected B vectors in the DHN are presumably along the twisting IR filaments. The linear polarization degree of the DHN is as large as p = 10%, and reaches p = 15% ± 2% at the radio polarization peak of the DHN. This means that the DHN has highly ordered magnetic field with synchrotron-emitting relativistic electrons.

Availability note (English)

Available from http://dx.doi.org/10.1088/2041-8205/719/2/L177

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal Letters
Journal Volume
719
Journal Issue
2
Journal Page Range
p. L177-L180
ISSN
2041-8205

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42045864
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ELECTRONS; FARADAY EFFECT; GALAXIES; GALAXY NUCLEI; MAGNETIC FIELDS; NEBULAE; POLARIZATION; RELATIVISTIC RANGE; SUPERNOVA REMNANTS; TELESCOPES
Descriptors DEC
COSMIC RADIO SOURCES; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; LEPTONS