NSV 22840

CONFIRMED MILKY WAY
 
Constellation
Ophiucus
Equatorial coordinates
α = 17 35 58.474
δ = -28 49 54.228
Galactic coordinates
l = 358.9699°
b = 1.8460°

Suspected 2013Ref
Confirmed 2013Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts -

Identifiers

NSV 22840 IRAS - GSC2.4.2 S8DS005010 AAVSO -
SIMBAD Terz V 2687 Pan-STARRS 73402639936402260 SAO - VSX 61275
GAIA DR3 4060313750650464512 SkyMapper 173558.48-284954.0 WRAY - GCVS -
2MASS J17355846-2849540 HIP - Hen - BD -
WISE J173558.47-284954.1 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) - Belzcyński et al. (2001) -
Gaposchkin (1957) - Kenyon (1986) - Akras et al. (2019) NSV 22840 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) -

Position

Right ascension (°) 263.9936Ref Parallax (mas) 0.004±0.076Ref Reddening E(B-V) (mag) 1.64±0.12Ref, Note
Declination (°) -28.8317Ref Distance (kpc) 8.52Ref, Note, 5.62Ref, Note    
Galactic longitude (°) 358.9699Ref Proper motion in α (mas/yr) 4.45±0.09Ref    
Galactic latitude (°) 1.8460Ref Proper motion in δ (mas/yr) -5.47±0.06Ref    

Observations

X-Ray NoRef IR type SRef Radio -
X-Ray type - J (mag) 10.50Ref Flickering -
GALEX FUV (mag) - H (mag) 9.20Ref Outbursts -
GALEX NUV (mag) - K (mag) 8.65Ref Outburst type -
IUE NoRef WISE W1 (mag) 8.21Ref Jets -
FUSE NoRef WISE W2 (mag) 8.19Ref Resolved nebula -
U (mag) - WISE W3 (mag) 7.63Ref IPmax (eV) 54.4Ref
B (mag) - WISE W4 (mag) 7.10Ref [O III] lines YesRef
V (mag) 17.70Ref IRAS 12μm (Jy) - He II lines YesRef
R (mag) 15.80Ref IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) - IRAS 60μm (Jy) - O VI lines NoRef
BP (mag) 17.36Ref IRAS 100μm (Jy) -
G (mag) 15.01Ref AKARI S09 (Jy) -
RP (mag) 13.55Ref AKARI S18 (Jy) -

Orbit

Orbital period (days) - 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 Yes?Ref     Mass ratio -
Orbital ephemeris -        

Cool component

Spectral type M0-3Ref Mass (M) - Pulsation YesRef
Eff. temperature (K) - Radius (R) - Type SRRef
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) 55000Ref        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

The spectrum of this star confirms its S-type symbiotic nature, and the OGLE-IV light curve reveals potential eclipse in addition to semi-regular pulsations, as detailed in Miszalski et al. (2013).


References

  • Miszalski, B., Mikołajewska, J., Udalski, A., 2013, MNRAS, 432, 4, 3186, 2013MNRAS.432.3186M


Last updated: November 5, 2019