G28.6−0.1 ADS: search title/keyword/abstract or fulltext

• Right Ascension: 18 43 55
• Declination: −03 53
• Size (/arcmin): 13×9
• Type: S
• Flux density at 1 GHz (/Jy): 3?
• Spectral Index: ?

Radio: Poorly defined regions of non-thermal emission.

X-ray: Diffuse shell, with thermal and non-thermal emission.

Point sources: Pulsar in NE.

Distance: HI absorption and CO suggests 9.6 kpc.

References:

• Helfand et al. 1989, ApJ, 341, 151. VLA at 1.4 GHz (15″) and 5 GHz (15″). ADS
• Bamba et al. 2001, PASJ, 53, L21. ASCA observations. ADS
• Ueno et al. 2003, ApJ, 588, 338. Chandra observations. ADS
• Ebisawa et al. 2005, ApJ, 635, 214. Chandra observations. ADS
• Zyuzin et al. 2018, MNRAS, 476, 2177. Pulsar observations. ADS
• Ranasinghe & Leahy 2018, MNRAS, 477, 2243. VGPS HI absorption, plus CO observations. ADS
• Lee et al. 2019, AJ, 157, 123. [FeII] IR observations. ADS
• Devin et al. 2021, A&A, 647, A68. Fermi observations. ADS
• Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18″: S=1.2 Jy) including polarisation, and Spitzer observations. ADS
• Castelletti et al. 2021, A&A, 653, A62.VLA 74-MHz survey flux density, and other low-frequency radio flux densities. ADS
• Sofue et al. 2021, ApJS, 253, 17. Nobeyama 45-m CO observations (20″) of region. ADS
• Amenomori et al. 2022, ApJ, 932, 120. γ-ray observations. ADS
• Dokara et al. et al. 2023, A&A, 671, A145. VLA and Effelsberg 100-m at 6 GHz, including polarisation, plus other radio flux densities. ADS

Last updated: 19 Mar 2024

home | documentation | detailed listings | summary listings

Dave Green / Cambridge, UK /