AX Per

CONFIRMED MILKY WAY
 
Constellation
Perseus
Equatorial coordinates
α = 01 36 22.697
δ = +54 15 02.318
Galactic coordinates
l = 129.5333°
b = -8.0441°

Suspected 1932Ref
Confirmed 1932Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts YesRef - Z AndRef

Identifiers

AX Per IRAS 01331+5359 GSC2.4.2 NAJZ000050 AAVSO 000-BBD-098
SIMBAD V* AX Per Pan-STARRS 173100240943441658 SAO - VSX 25601
GAIA DR3 409028569033785728 SkyMapper - WRAY - GCVS AX Per
2MASS J01362271+5415023 HIP - Hen - BD -
WISE J013622.71+541502.5 TYC 3671-247-1 ESO - HD -

Symbiotic Catalogs

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

Position

Right ascension (°) 24.0946Ref Parallax (mas) 0.424±0.030Ref Reddening E(B-V) (mag) 0.19±0.01Ref, Note
Declination (°) 54.2506Ref Distance (kpc) 2.5Ref, 1.7Ref
2.11Ref, Note, 2.13Ref, Note
   
Galactic longitude (°) 129.5333Ref Proper motion in α (mas/yr) -1.83±0.03Ref    
Galactic latitude (°) -8.0441Ref Proper motion in δ (mas/yr) -5.86±0.03Ref    

Observations

X-Ray NoRef IR type SRef Radio YesRef
X-Ray type - J (mag) 6.60Ref Flickering NoRef, Yes?Ref
GALEX FUV (mag) - H (mag) 5.69Ref Outbursts YesRef
GALEX NUV (mag) - K (mag) 5.35Ref Outburst type Z AndRef
IUE YesRef WISE W1 (mag) 5.27Ref Jets -
FUSE NoRef WISE W2 (mag) 5.17Ref Resolved nebula NoRef
U (mag) - WISE W3 (mag) 4.96Ref IPmax (eV) 99.0Ref, 109.3Ref
B (mag) 12.57Ref WISE W4 (mag) 4.42Ref [O III] lines YesRef
V (mag) 11.10Ref IRAS 12μm (Jy) 0.28Ref He II lines YesRef
R (mag) 11.04Ref IRAS 25μm (Jy) 0.25Ref [Fe VII] lines YesRef
I (mag) - IRAS 60μm (Jy) 0.40Ref O VI lines NoRef
BP (mag) 11.23Ref IRAS 100μm (Jy) 2.04Ref
G (mag) 9.89Ref AKARI S09 (Jy) 0.55Ref
RP (mag) 8.70Ref AKARI S18 (Jy) 0.17Ref

Orbit

Orbital period (days) 681.6Ref, 680.8±0.2Ref,
682.1±1.4Ref
γ velocity (km/h) -116.5±0.4Ref, -117.44±0.14Ref Size of giant’s orbit (AU) 0.49Ref
Eccentricity 0±nanRef RV of giant (km/h) 7.5±0.9Ref, 7.78±0.21Ref Separation (AU) -
Inclination (°) 70±3Ref, 90±6Ref Inferior conj. of giant (JD) 2451134.3 Mass function 0.0333Ref
Eclipses YesRef     Mass ratio 2.5Ref, 2.3Ref
Orbital ephemeris Min (pg) = 2436679.4 + 681.6 x ERef, Min (V) = 2436667±3 + 680.8±0.2 x ERef        

Cool component

Spectral type M5.2 IIIRef, M4.5 IIIRef,
M5.5 IIIRef
Mass (M) 3Ref, 1Ref,
0.9±0.2Ref
Pulsation -
Eff. temperature (K) 3300Ref, 3400±150Ref,
3320Ref
Radius (R) 102±3Ref, 115±2Ref Type -
IR type SRef Luminosity (L) 3000Ref, 1800Ref,
1200±400Ref, 1450Ref
Pulsation period (days) -
Metallicity [Fe/H] -0.26±0.1Ref     Pulsation ephemeris -

Hot component

Type/Spectral type - Mass (M) 0.6Ref, 0.4Ref,
0.37±0.06Ref
Spin period (min) -
Shell-burning/Accreting-only shell-burningRef Radius (R) 0.08Ref, 0.065Ref Accretion disk -
Eff. temperature (K) 120000Ref, 105000Ref,
115000-170000Ref
Luminosity (L) 240-310Ref, 710Ref,
360Ref, 380Ref
   
Lower limit (K) -        
Upper limit (K) -        

Links

SIMBAD   CDS Portal   ARAS Database


Notes

The star was discovered by Merrill & Humason (1932), and they reported an "anomalous combination in a single spectrum of features which ordinarily occur near opposite ends of the sequence of stellar temperatures." The detection of TiO bands and a strong He II line was reported by Merrill & Burwell (1933). For historical light curves, you can refer to, e. g., Skopal et al. (2001) and Mártonfi et al. (2021).


References


Last updated: January 12, 2024