Terz V 2513

CONFIRMED MILKY WAY
 
Constellation
Ophiucus
Equatorial coordinates
α = 17 33 47.261
δ = -27 19 26.425
Galactic coordinates
l = 359.9792°
b = 3.0664°

Suspected 2014Ref
Confirmed 2014Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts YesRef - SyN or Z AndRef

Identifiers

Terz V 2513 IRAS - GSC2.4.2 S8DU406960 AAVSO -
SIMBAD Terz V 2513 Pan-STARRS 75212634470741334 SAO - VSX 61016
GAIA DR3 4061345440525803776 SkyMapper 173347.31-271927.1 WRAY - GCVS -
2MASS J17334728-2719266 HIP - Hen - BD -
WISE J173347.31-271927.4 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) - Belzcyński et al. (2001) -
Gaposchkin (1957) - Kenyon (1986) - Akras et al. (2019) 2MASSJ17334728-2719266 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) -

Position

Right ascension (°) 263.4469Ref Parallax (mas) -0.287±0.129Ref Reddening E(B-V) (mag) 1.58±0.05Ref, Note
Declination (°) -27.3240Ref Distance (kpc) 9.27Ref, Note, 6.70Ref, Note    
Galactic longitude (°) 359.9792Ref Proper motion in α (mas/yr) -2.10±0.16Ref    
Galactic latitude (°) 3.0664Ref Proper motion in δ (mas/yr) -10.03±0.11Ref    

Observations

X-Ray NoRef IR type SRef Radio -
X-Ray type - J (mag) 9.32Ref Flickering -
GALEX FUV (mag) - H (mag) 7.91Ref Outbursts YesRef
GALEX NUV (mag) - K (mag) 7.26Ref Outburst type SyN or Z AndRef
IUE NoRef WISE W1 (mag) 6.32Ref Jets -
FUSE NoRef WISE W2 (mag) 5.87Ref Resolved nebula -
U (mag) - WISE W3 (mag) 4.73Ref IPmax (eV) 54.4Ref
B (mag) - WISE W4 (mag) 4.03Ref [O III] lines YesRef
V (mag) - IRAS 12μm (Jy) - He II lines YesRef
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) - IRAS 60μm (Jy) - O VI lines NoRef
BP (mag) 16.59Ref IRAS 100μm (Jy) -
G (mag) 14.85Ref AKARI S09 (Jy) 0.54Ref
RP (mag) 12.51Ref AKARI S18 (Jy) 0.33Ref

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 -     Mass ratio -
Orbital ephemeris -        

Cool component

Spectral type M2Ref 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


Notes

An increase of up to 5.0 magnitudes was observed, that could be attributed to either a Z And outburst or a symbiotic nova outburst, as discussed in Miszalski & Mikołajewska (2014).


References


Last updated: May 11, 2021