G8.7−0.1
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(W30)
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- Right Ascension: 18 05 30
- Declination: −21 26
- Size (/arcmin): 45
- Type: S?
- Flux density at 1 GHz (/Jy): 80
- Spectral Index: 0.5
Notes: Has been called G8.6−0.1.
- Radio: Clumpy non-thermal shell, with low-frequency turnover.
- X-ray: Northern edge detected.
- Point sources: Pulsar inside W edge.
- Distance: Optical extinction suggests 4.2 kpc.
References:
- Odegard 1986, AJ, 92, 1372. TPT at 57.5 MHz (7.′2×9.′7: S=190±50 Jy).
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- Kassim & Weiler 1990, Nature, 343, 146. VLA at 327 MHz (3.′0×3.′7).
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- Kassim & Weiler 1990, ApJ, 360, 184. VLA at 327 MHz (2.′8×4.′1: S=129±11 Jy), and part at 1.4 GHz (0.′9×1.′8), plus review of flux densities.
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- Frail et al. 1994, AJ, 107, 1120. VLA at 327 MHz (37″×55″).
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- Finley & Ögelman 1994, ApJ, 434, L25. ROSAT observations, including pulsar.
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- Aharonian et al. 2005, Science, 307, 1938. H.E.S.S. detection.
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- Aharonian et al. 2006, ApJ, 636, 777. H.E.S.S. observations.
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- Landi et al. 2006, ApJ, 651, 190. X-ray observations.
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- Briskin et al. 2006, ApJ, 652, 554. Pulsar proper motion.
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- Hewitt & Yusef-Zadeh 2009, ApJ, 694, L16. OH maser detection.
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- Castro & Slane 2010, ApJ, 717, 372. Fermi observations.
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- Ajello et al. 2012, ApJ, 744, 80. Fermi observations.
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- Pihlström et al. 2014, AJ, 147, 73. VLA search for methanol masers.
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- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
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- Lee et al. 2019, AJ, 157, 123. [FeII] IR observations.
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- Wang et al. 2020, A&A, 639, A72. Optical extinction for distance.
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- Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18″) including polarisation, and Spitzer observations.
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Last updated: 20 Dec 2022
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