V2428 Cyg

CONFIRMED MILKY WAY
 
Constellation
Cygnus
Equatorial coordinates
α = 20 41 19.016
δ = +34 44 52.226
Galactic coordinates
l = 75.9428°
b = -4.4407°

Suspected 1974Ref
Confirmed 1983Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts YesRef

Identifiers

V2428 Cyg IRAS - GSC2.4.2 N347099190 AAVSO 000-BFR-583
SIMBAD V* V2428 Cyg Pan-STARRS 149693103291648015 SAO - VSX 137537
GAIA DR3 1870194997404105856 SkyMapper - WRAY - GCVS V2428 Cyg
2MASS J20411901+3444522 HIP - Hen 2-468 BD -
WISE J204119.01+344452.2 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) He2-468 (Conf.) Belzcyński et al. (2001) Hen 2-468 (Conf.)
Gaposchkin (1957) - Kenyon (1986) He2-468 (Conf.) Akras et al. (2019) Hen 2-468 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) VDS 175 (Conf.)

Position

Right ascension (°) 310.3292Ref Parallax (mas) 0.096±0.022Ref Reddening E(B-V) (mag) 0.63±0.02Ref, Note
Declination (°) 34.7478Ref Distance (kpc) 8.20Ref, Note, 6.42Ref, Note    
Galactic longitude (°) 75.9428Ref Proper motion in α (mas/yr) -0.74±0.02Ref    
Galactic latitude (°) -4.4407Ref Proper motion in δ (mas/yr) -2.36±0.02Ref    

Observations

X-Ray YesRef IR type SRef Radio NoRef
X-Ray type βRef J (mag) 9.40Ref Flickering -
GALEX FUV (mag) - H (mag) 8.31Ref Outbursts YesRef
GALEX NUV (mag) - K (mag) 7.95Ref Outburst type -
IUE NoRef WISE W1 (mag) 7.78Ref Jets -
FUSE NoRef WISE W2 (mag) 7.85Ref Resolved nebula NoRef
U (mag) - WISE W3 (mag) 7.50Ref IPmax (eV) 114Ref
B (mag) 16.46Ref WISE W4 (mag) 7.11Ref [O III] lines NoRef
V (mag) 14.73Ref IRAS 12μm (Jy) - He II lines YesRef
R (mag) 14.21Ref IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) - IRAS 60μm (Jy) - O VI lines YesRef
BP (mag) 14.19Ref IRAS 100μm (Jy) -
G (mag) 12.57Ref AKARI S09 (Jy) -
RP (mag) 11.43Ref AKARI S18 (Jy) -

Orbit

Orbital period (days) 774Ref γ velocity (km/h) - Size of giant’s orbit (AU) -
Eccentricity - RV of giant (km/h) - Separation (AU) -
Inclination (°) - Inferior conj. of giant (JD) - Mass function -
Eclipses -     Mass ratio -
Orbital ephemeris Max (B) = 2440749 + 774 x ERef        

Cool component

Spectral type MRef Mass (M) - Pulsation -
Eff. temperature (K) - Radius (R) - Type -
IR type SRef Luminosity (L) - Pulsation period (days) -
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

Type/Spectral type - Mass (M) - Spin period (min) -
Shell-burning/Accreting-only shell-burningRef Radius (R) - Accretion disk -
Eff. temperature (K) - Luminosity (L) -    
Lower limit (K) -        
Upper limit (K) -        

Links

SIMBAD   CDS Portal   ARAS Database


Notes

Initially classified as a PN, this object was suspected to have a symbiotic nature by Allen (1974). Subsequent observations by Carrasco et al. (1983) revealed strong H and He lines, a detectable stellar continuum, and O VI lines. Additionally, the object was detected in two outbursts, as reported in Munari & Jurdana-Šepić (2002) and Munari et al. (2014).


References


Last updated: April 8, 2022