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Watson et al. 1983, ApJ, 273, 688. X-ray observations. ... Kotani et al. 1996, PASJ, 48, 619. X-ray line emission from SS433.

to be radio nebula powered by a stellar wind (see Gaensler et al. ... Watson et al. 2003, Leto et al. 2009). G203.212.3, a optical ring about 3 arcmin in diameter, was reported as a possible SNR by Winkler & Reipurth (1992), but was

Anantharamaiah et al. 1991, MNRAS, 249, 262. VLA at 330 MHz (17''33''). ... LaRosa et al. 2000, AJ, 119, 207. VLA at 333 MHz (24''43'').

20 Feb 2023: G70.71.2, which was reported as a SNR by Reich et al. ... Watson et al.2003, Leto et al. 2009). • G203.2–12.3, a optical ring about 3 arcmin in diameter, was reported as a possible SNR by Winkler &Reipurth (1992), but

20 Feb 2023: G70.71.2, which was reported as a SNR by Reich et al. ... Watson et al. 2003, Leto et al. 2009). • G203.2–12.3, a optical ring about 3 arcmin in diameter, was reported as a possible SNR by Winkler & Reipurth(1992), but

10 Jan 2023: 1991, Nature, 350, 309. VLA of NH3 emission from. surroundings.Anantharamaiah et al. ... 1991, MNRAS, 249, 262. VLA at. 330 MHz (17′′33′′).Serabyn et al.

10 Jan 2023: 1991, MNRAS, 249, 262. VLA at 330 MHz. (17′′33′′).Serabyn et al. ... VLA of nearby. H2O masers.Yusef-Zadeh et al. 1999, ApJ, 512, 230.