RAW 1019

SUSPECTED SMC
 
Constellation
Tucana
Equatorial coordinates
α = 00 56 52.955
δ = -72 21 11.454
Galactic coordinates
l = 302.3508°
b = -44.7689°

Suspected 2002Ref
Confirmed -
Symbiotic IR type S?Ref
Hot component type -
Outbursts -

Identifiers

RAW 1019 IRAS - GSC2.4.2 S0WB232302 AAVSO -
SIMBAD RAW 1019 Pan-STARRS - SAO - VSX -
GAIA DR3 4689000897310347520 SkyMapper 005652.96-722111.3 WRAY - GCVS -
2MASS J00565295-7221115 HIP - Hen - BD -
WISE J005652.95-722111.4 TYC - ESO - HD -

Symbiotic Catalogs

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

Position

Right ascension (°) 14.2206Ref Parallax (mas) -0.047±0.026Ref Reddening E(B-V) (mag) 0.38±0.01Ref, Note
Declination (°) -72.3532Ref Distance (kpc) 62.1±1.9Ref
23.64Ref, Note, 17.07Ref, Note
   
Galactic longitude (°) 302.3508Ref Proper motion in α (mas/yr) 0.71±0.03Ref    
Galactic latitude (°) -44.7689Ref Proper motion in δ (mas/yr) -1.29±0.03Ref    

Observations

X-Ray NoRef IR type S?Ref Radio -
X-Ray type - J (mag) 13.21Ref Flickering -
GALEX FUV (mag) - H (mag) 12.35Ref Outbursts -
GALEX NUV (mag) - K (mag) 12.04Ref Outburst type -
IUE NoRef WISE W1 (mag) 11.72Ref Jets -
FUSE NoRef WISE W2 (mag) 11.86Ref Resolved nebula -
U (mag) 19.50Ref WISE W3 (mag) 11.70Ref IPmax (eV) No linesRef
B (mag) 18.14Ref WISE W4 (mag) 8.80Ref [O III] lines NoRef
V (mag) 16.19Ref IRAS 12μm (Jy) - He II lines NoRef
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) 14.38Ref IRAS 60μm (Jy) - O VI lines NoRef
BP (mag) 16.66Ref IRAS 100μm (Jy) -
G (mag) 15.61Ref AKARI S09 (Jy) -
RP (mag) 14.61Ref 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 -     Mass ratio -
Orbital ephemeris -        

Cool component

Spectral type CRef Mass (M) - Pulsation -
Eff. temperature (K) 3700Ref Radius (R) - Type -
IR type S?Ref Luminosity (L) 3572±257Ref Pulsation period (days) -
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

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

Links

SIMBAD   CDS Portal


Notes

Included in the list of possible symbiotic stars or closely related objects in Munari & Zwitter (2002), this star has been classified as a carbon star in Rebeirot et al. (1993). It is also labeled as an anomalous oxygen-rich AGB star in Boyer et al. (2011). Additionally, Raimondo et al. (2005) reported variability with a period of 37.8 days.


References


Last updated: May 2, 2022