Published August 20, 2010
| Version v1
Journal article
HIGHLY POLARIZED COUNTERPART OF THE DOUBLE HELIX NEBULA
Creators
- 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/L177Additional 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