G39.7−2.0
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W50,
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SS433
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- Right Ascension: 19 12 20
- Declination: +04 55
- Size (/arcmin): 120×60
- Type: ?
- Flux density at 1 GHz (/Jy): 85?
- Spectral Index: 0.7?
Notes: Eastern part has been called G40.0−3.1. Is this a SNR?
- Radio: Elongated shell, containing SS433, adjacent to the HII region S74.
- Optical: Faint filaments at the edge of the radio emission.
- X-ray: Emission from SS433 and two lobes.
- Point sources: SS433 is the compact source in the centre of the W50.
- Distance: HI absorption and CO observations indicate 4.9 kpc, optical emission gives 4.7 kpc.
References:
- van den Bergh 1980, ApJ, 236, L23. Optical in Hα and [SII].
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- Zealey et al. 1980, MNRAS, 192, 731. Optical spectra.
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- van Gorkom et al. 1982, MNRAS, 198, 757. WSRT HI absorption to nearby point source (not SS433).
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- Seaquist & Gilmore 1982, AJ, 87, 378. VLA observations of nearby source.
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- Watson et al. 1983, ApJ, 273, 688. X-ray observations.
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- Downes et al. 1986, MNRAS, 218, 393. Effelsberg 100-m at 4.75 GHz (2.′4: S=34±4 Jy), plus previous 1.7 and 2.7 GHz data.
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- Romney et al. 1987, ApJ, 321, 822. VLBI of SS433, including distance.
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- Elston & Baum 1987, AJ, 94, 1633. Mosaic with VLA at 1.4 GHz (30″) of fine structure only.
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- Kawai et al. 1989, PASJ, 41, 491. X-ray observations of SS433.
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- Band 1989, ApJ, 336, 937. Einstein and EXOSAT observations.
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- Yamauchi et al. 1994, PASJ, 46, L109. X-ray spectral observations.
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- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
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- Brinkmann et al. 1996, A&A, 312, 306. ROSAT observations.
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- Kotani et al. 1996, PASJ, 48, 619. X-ray line emission from SS433.
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- Safi-Harb & Ögelman 1997, ApJ, 483, 868. ROSAT observations.
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- Dubner et al. 1998, AJ, 116, 1842. VLA at 328 MHz (60″×64″: S=160±20 Jy), and 1.4 GHz (54″×56″), plus NRAO 140-ft at 1.4 GHz (21′) for HI observations.
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- Safi-Harb & Petre 1999, ApJ, 512, 784. X-ray observations.
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- Aharonian et al. 2001, A&A, 375, 1008. H.E.S.S. limit.
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- Brinkmann et al. 2007, A&A, 463, 611. XMM-Newton observations of E lobe.
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- Boumis et al. 2007, MNRAS, 381, 308. Optical observations.
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- Lockman et al. 2007, MNRAS, 381, 881. HI observations.
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- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.′5: S=37±4 Jy), including polarisation and review of flux densities.
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- Farnes et al. 2017, MNRAS, 467, 4777. ATCA at 1.4 to 3.1 GHz, including polarisation and Hα observations.
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- Broderick et al. 2018, MNRAS, 475, 5360. LOFAR at 115 to 189 MHz, including 140 MHz (55″×78″).
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- Su et al. 2018, ApJ, 863, 103. CO and HI observations.
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- Sun et al. 2019, A&A, 626, A113. Fermi observations.
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- Liu et al. 2020, ApJ, 892, 143. CO and CN observations of W edge.
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- Rosado et al. 2021, MNRAS, 506, 4263. Optical spectroscopy, including distance.
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- Hayakawa et al. 2022, PASJ, 74, 510. Chandra observations of E.
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- Kayama et al. 2022, PASJ, 74, 1143. Chandra observations.
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- Safi-Harb et al. 2022, ApJ, 935, 163. NuSTAR, Chandra and XMM-Newton observations.
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Last updated: 4 Jan 2024
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