Binary star system in the constellation Aquila
SS 433
SS 433 at the centre of
supernova remnant W50 Credit :
NRAO/AUI/NSF, K. Golap, M. Goss; NASA’s Wide Field Survey Explorer (WISE)
Observation dataEpoch J2000.0 Equinox J2000.0 (ICRS )
Constellation
Aquila
Right ascension
19h 11m 49.56s [ 1]
Declination
+04° 58′ 57.8″[ 1]
Apparent magnitude (V)
13.0 - 17.3[ 2]
Characteristics
Spectral type
A7Ib
Variable type
Eclipsing binary [ 2]
Astrometry Proper motion (μ) RA: −3.027[ 1] mas /yr Dec.: −4.777[ 1] mas /yr Parallax (π)0.1182± 0.0233 mas [ 1] Distance 18,000± 700 ly ( 5,500± 200[ 3] [ 4] pc )
Orbit [ 5] Period (P)13.082 d Eccentricity (e)0.05 ± 0.01 Inclination (i)79°
Other designations V1343 Aql, GAL 039.7-02.0, 2MASS J19114957+0458578, USNO 659, 1A 1909+04, 87GB 190920.8+045332, NEK 40.1-02.1, 3A 1909+048, GPS 1909+049, RGB J1911+049, BWE 1909+0453, GRS 039.60 -01.80, RX J1911.7+0459, 4C 04.66, 1H 1908+047, 1RXS J191149.7+045857, 2E 1909.3+0453, HBHA 204-02, AAVSO 1906+04, 2E 4204, INTEGRAL1 110, TXS 1909+048, 1ES 1909+04.8, INTREF 969, 4U 1908+05.
Database references SIMBAD data
SS 433 is a microquasar or eclipsing X-ray binary system , consisting of a stellar-mass black hole accreting matter from an A-type companion star .[ 5] [ 6] SS 433 is the first discovered microquasar.[ 7] It is at the centre of the supernova remnant W50 .
SS 433's designation comes from the initials of two astronomers at Case Western Reserve University : Nicholas Sanduleak and Charles Bruce Stephenson . It was the 433rd entry in their 1977 catalog of stars with strong emission lines.[ 7] Its emission lines were studied by Mordehai Milgrom in 1979.[ 8]
^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties" . Astronomy and Astrophysics . 674 : A1. arXiv :2208.00211 . Bibcode :2023A&A...674A...1G . doi :10.1051/0004-6361/202243940 . S2CID 244398875 .
Gaia DR3 record for this source at VizieR .
^ a b Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S . 1 : B/gcvs. Bibcode :2009yCat....102025S .
^ Blundell, Katherine M. ; Bowler, Michael G. (2004). "Symmetry in the Changing Jets of SS 433 and Its True Distance from Us". The Astrophysical Journal . 616 (2): L159 – L162 . arXiv :astro-ph/0410456 . Bibcode :2004ApJ...616L.159B . doi :10.1086/426542 . ISSN 0004-637X . S2CID 11213274 .
^ Jeffrey, Robert (2016). The remarkable outflows from the galactic microquasar SS433 . ora.ox.ac.uk (DPhil thesis). University of Oxford. EThOS uk.bl.ethos.730205 .
^ a b Cherepashchuk, A. M.; Belinski, A. A.; Dodin, A. V.; Postnov, K. A. (2021). "Discovery of orbital eccentricity and evidence for orbital period increase of SS433" . Monthly Notices of the Royal Astronomical Society: Letters . 507 (1): L19 – L23 . arXiv :2107.09005 . Bibcode :2021MNRAS.507L..19C . doi :10.1093/mnrasl/slab083 .
^ Hillwig, T. C.; Gies, D. R.; Huang, W.; McSwain, M. V.; Stark, M. A.; Van Der Meer, A.; Kaper, L. (2004). "Identification of the Mass Donor Star's Spectrum in SS 433". The Astrophysical Journal . 615 (1): 422– 431. arXiv :astro-ph/0403634 . Bibcode :2004ApJ...615..422H . doi :10.1086/423927 . S2CID 17930915 .
^ a b SS 433 , David Darling, entry in The Internet Encyclopedia of Science , accessed on line September 14, 2007.
^ Milgrom, Mordehai (October 1979). "Thomson scattered lines in the spectrum of SS 433 - A powerful tool for studying the system". Astronomy and Astrophysics . 78 (3): L17 – L20 . Bibcode :1979A&A....78L..17M .