W50 (nebula)

W50
Observation
W50
Other designations	SNR G039.7-02.0
Event type	Supernova remnant
Spectral class	II
Location
Constellation	Aquila
Right ascension	19^h 11^m 49^s
Declination	+04° 59′ 12′′
Epoch	J2000.0
Galactic coordinates	039.697 -02.241
Distance	18,000 Ly
Remnant	?
Characteristics
Notable features	central source: SS 433.
Energetics
Peak apparent magnitude	?
See also

W50 or SNR G039.7-02.0, once referred to as the Manatee Nebula,^[1] is a Supernova remnant located in the constellation Aquila, about 18,000 light years away. In its centre lies the micro-quasar SS 433, whose jets are distorting the remnant's shell. Most likely W50 and SS 433 are related objects, remnants from a supernova which occurred about 20,000 years ago.^[1]

Notes

1 2 "IMAGE RELEASE: A Microquasar Makes a Giant Manatee Nebula". National Radio Astronomy Observatory. 19 Jan 2013. Retrieved 20 Jan 2013.

References

Database references
Simbad	data

SAFI-HARB S.; DUROUCHOUX P.; PETRE R. (2001). "The galactic microquasar W 50 / SS 433 system.". Astrophys. Space Sci. Suppl. 276: 133–134. Bibcode:2001ApSSS.276..133S. doi:10.1023/A:1011610421644.
VELAZQUEZ P.F.; RAGA A.C. (2000). "A numerical simulation of the W50-SS 433 system". Astronomy & Astrophysics. 362: 780–785. Bibcode:2000A&A...362..780V.
SAFI-HARB S.; PETRE R. (1999). "Rossi X-ray timing explorer observations of the eastern lobe of W50 associated with SS 433". The Astrophysical Journal. 512 (2): 784–792. Bibcode:1999ApJ...512..784S. doi:10.1086/306803.
DUBNER G.M.; HOLDAWAY M.; GOSS W.M.; MIRABEL I.F. (1998). "A high-resolution radio study of the W50-SS 433 system and the surrounding medium". The Astrophysical Journal. 116 (4): 1842–1855. Bibcode:1998AJ....116.1842D. doi:10.1086/300537.
SAFI-HARB S.; OEGELMAN H. (1996). "ROSAT and ASCA observations of the X-ray lobes of W 50 associated with the semi-relativistic two-sided jets source: SS 433". Bull. Am. Astron. Soc. 28: 954. Bibcode:1996BAAS...28W.954S.
MURATA K.; SHIBAZAKI N. (1996). "Interaction of jets with a supernova remnant in the SS 433/W50 system". Publ. Astron. Soc. Jap. 48: 819–825. Bibcode:1996PASJ...48..819M. doi:10.1093/pasj/48.6.819.
YAMAUCHI S.; KAWAI N.; AOKI T. (1994). "A non-thermal X-ray spectrum from the supernova remnant W 50". Publ. Astron. Soc. Jap. 46: L109–L113. Bibcode:1994PASJ...46L.109Y.
ELSTON R.; BAUM S. (1987). "High-resolution radio observations of W 50, the remnant associated with SS 433". The Astrophysical Journal. 94: 1633–1640. Bibcode:1987AJ.....94.1633E. doi:10.1086/114594.
GOSACHINSKIJ I.V.; KHERSONSKIJ V.K. (1986). "Neutral hydrogen in the vicinity of the supernova remnant W 50". Astrofizika. 25: 287–295. Bibcode:1986Afz....25..287G.
DOWNES A.J.B.; PAULS T.; SALTER C.J. (1986). "The supernova remnant W 50 at 5 GHz". Mon. Not. R. Astron. Soc. 218: 393–407. Bibcode:1986MNRAS.218..393D. doi:10.1093/mnras/218.3.393.
MAZEH T.; AGUILAR L.A.; TREFFERS R.R.; KOENIGL A.; et al. (1983). "Kinematics of the optical filaments in W 50". The Astrophysical Journal. 265: 235–238. Bibcode:1983ApJ...265..235M. doi:10.1086/160668.
HUANG Y.-L.; DAME T.M.; THADDEUS P. (1983). "A large molecular cloud toward the SNR W50 and SS 433". The Astrophysical Journal. 272: 609–614. Bibcode:1983ApJ...272..609H. doi:10.1086/161323.
ZAVALA J.; VELAZQUEZ P.F.; CERQUEIRA A.H.; DUBNER G.M. (2008). "Three-dimensional hydrodynamical simulations of the large-scale structure of W50-SS433". Mon. Not. R. Astron. Soc. 387 (2): 839–844. Bibcode:2008MNRAS.387..839Z. doi:10.1111/j.1365-2966.2008.13281.x.
BOUMIS P.; MEABURN J.; ALIKAKOS J.; REDMAN M.P.; et al. (2007). "Deep optical observations of the interaction of the SS 433 microquasar jet with the W50 radio continuum shell". Mon. Not. R. Astron. Soc. 381: 308–318. arXiv:0707.4243. Bibcode:2007MNRAS.381..308B. doi:10.1111/j.1365-2966.2007.12276.x.
MOLDOWAN A.; SAFI-HARB S. (2005). "Chandra and RXTE study of the western lobe of W 50 and galactic microquasar SS 433". J. R. Astron. Soc. Can. 99: 141–141. Bibcode:2005JRASC..99S.141M.

External links

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