Note: this is
an archived version which has been superseded. The current SNR
catalogue is at
https://www.mrao.cam.ac.uk/surveys/snrs/
G106.3+2.7
ADS: search fulltext or
title/keyword/abstract
- Right Ascension: 22 27 30
- Declination: +60 50
- Size (/arcmin): 60×24
- Type: C?
- Flux density at 1 GHz (/Jy): 6
- Spectral Index: 0.6
Notes: Incorporates the pulsar wind nebula G106.6+2.9 (the `Boomerang').
- Radio: Faint extended source, which brighter `head' to NE.
- X-ray: Pulsar and wind nebula.
- Point sources: Pulsar.
References:
- Pineault & Joncas 2000, AJ, 120, 3218. DRAO at 408 MHz (3.'5×3.'9: S=10.5±0.3 Jy) and 1.4 GHz (1.'0×1.'2: S=4.9±0.6 Jy), plus HI.
ADS
- Halpern et al. 2001, ApJ, 547, 323. X-ray and radio observations of the `head'.
ADS
- Halpern et al. 2001, ApJ, 552, L125. Pulsar detection.
ADS
- Kothes et al. 2001, ApJ, 560, 236. CGPS at 1.4 GHz, including HI, plus CO and other observations.
ADS
- Ng & Romani 2004, ApJ, 601, 479. Chandra detection of pulsar wind nebula.
ADS
- Kothes et al. 2004, ApJ, 607, 855. HI polarisation absorption.
ADS
- Kothes et al. 2006, ApJ, 638, 225. Effelsberg 100-m at 4.85 (2.'4), 8.35 (1.'4), 10.5 (1.'2) and 32 GHz (0.'45) of pulsar wind nebula, including polarisation.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=8.6±1.0 Jy) and 1420 MHz (~1': S=4.8±0.5 Jy), including polarisation and review of flux densities.
ADS
- Abdo et al. 2007, ApJ, 664, L91. γ-ray observations.
ADS
- Casandjian & Grenier 2008, A&A, 489, 849. γ-ray observations.
ADS
- Acciari et al. 2009, ApJ, 703, L6. γ-ray observations.
ADS
- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.'5: S=2.0±0.3 Jy), including polarisation and review of flux densities.
ADS
- Xin et al. 2019, ApJ, 885, 162. Fermi observations.
ADS
- Albert et al. 2020, ApJ, 896, L29. γ-ray observations.
ADS
- Fujita et al. 2021, ApJ, 912, 133. Suzaku observations.
ADS
- Tibet ASγ Collaboration: Amenomori et al. 2021, NatAs, 5, 460. High energy γ-ray observations.
ADS
- Ge et al. 2021, The Innovation, 2, 100118. Chandra and XMM-Newton observations.
ADS
Last updated: 16 Dec 2022
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