CONFIRMED
MILKY WAY
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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 - |
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.) |
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 |
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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 |
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 |
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 |
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 | - |
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 |
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Lower limit (K) | - | ||||
Upper limit (K) | - |
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).