[MMU2013] 001.71+01.14

LIKELY MILKY WAY
 
Constellation
Sagittarius
Equatorial coordinates
α = 17 45 13.665
δ = -26 52 43.005
Galactic coordinates
l = 1.7108°
b = 1.1465°

Suspected 2013Ref
Confirmed -
Symbiotic IR type S?Ref
Hot component type shell-burning?Ref
Outbursts -

Identifiers

[MMU2013] 001.71+01.14 IRAS - GSC2.4.2 S8E4350685 AAVSO -
SIMBAD 2MASS J17451367-2652427 Pan-STARRS 75742663069025990 SAO - VSX 305992
GAIA DR3 4060829013611693952 SkyMapper - WRAY - GCVS -
2MASS J17451367-2652427 HIP - Hen - BD -
WISE J174513.66-265242.8 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) - Belzcyński et al. (2001) -
Gaposchkin (1957) - Kenyon (1986) - Akras et al. (2019) 001.71+01.14 (Susp.)
Boyarchuk (1969) - Vaidis (1988, 1991) -

Position

Right ascension (°) 266.3069Ref Parallax (mas) -0.191±0.117Ref Reddening E(B-V) (mag) 2.97±0.28Ref, Note
Declination (°) -26.8786Ref Distance (kpc) 9.76Ref, Note, 8.86Ref, Note    
Galactic longitude (°) 1.7108Ref Proper motion in α (mas/yr) -1.82±0.15Ref    
Galactic latitude (°) 1.1465Ref Proper motion in δ (mas/yr) -9.18±0.09Ref    

Observations

X-Ray NoRef IR type S?Ref Radio -
X-Ray type - J (mag) 10.28Ref Flickering -
GALEX FUV (mag) - H (mag) 8.75Ref Outbursts -
GALEX NUV (mag) - K (mag) 7.94Ref Outburst type -
IUE NoRef WISE W1 (mag) 7.62Ref Jets -
FUSE NoRef WISE W2 (mag) 7.70Ref Resolved nebula -
U (mag) - WISE W3 (mag) 7.41Ref IPmax (eV) 24.6Ref
B (mag) - WISE W4 (mag) 6.65Ref [O III] lines NoRef
V (mag) - IRAS 12μm (Jy) - He II lines NoRef
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) - IRAS 60μm (Jy) - O VI lines NoRef
BP (mag) 20.25Ref IRAS 100μm (Jy) -
G (mag) 16.65Ref AKARI S09 (Jy) -
RP (mag) 14.89Ref 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 M6Ref Mass (M) - Pulsation YesRef
Eff. temperature (K) - Radius (R) - Type SRRef
IR type S?Ref 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-burning?Ref Radius (R) - Accretion disk -
Eff. temperature (K) - Luminosity (L) -    
Lower limit (K) 25000Ref        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

The symbiotic nature is supported by the analysis of Akras et al. (2019).


References

  • Akras, S., Leal-Ferreira, M. L., Guzman-Ramirez, L. et al., 2019, MNRAS, 483, 4, 5077, 2019MNRAS.483.5077A
  • Miszalski, B., Mikołajewska, J., Udalski, A., 2013, MNRAS, 432, 4, 3186, 2013MNRAS.432.3186M


Last updated: November 5, 2019