CONFIRMED
MILKY WAY
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CI Cyg | IRAS 19483+3533 | GSC2.4.2 N2FW001083 | AAVSO 000-BCJ-172 |
SIMBAD V* CI Cyg | Pan-STARRS 150822975494761356 | SAO - | VSX 11030 |
GAIA DR3 2047647756007944576 | SkyMapper - | WRAY - | GCVS CI Cyg |
2MASS J19501182+3541029 | HIP 97594 | Hen 3-1784 | BD - |
WISE J195011.82+354103.0 | TYC 2681-154-1 | ESO - | HD - |
Bidelman (1954) | CI Cyg (Conf.) | Allen (1984) | CI Cyg (Conf.) | Belzcyński et al. (2001) | CI Cyg (Conf.) |
Gaposchkin (1957) | CI Cyg (Conf.) | Kenyon (1986) | CI Cyg (Conf.) | Akras et al. (2019) | CI Cyg (Conf.) |
Boyarchuk (1969) | CI Cyg (Conf.) | Vaidis (1988, 1991) | CI Cyg (Conf.) |
Right ascension (°) | 297.5493Ref | Parallax (mas) | 0.476±0.025Ref | Reddening E(B-V) (mag) | 0.44±0.03Ref, Note |
Declination (°) | 35.6842Ref | Distance (kpc) | 2-2.6Ref, 2Ref, 2Ref 1.94Ref, Note, 1.86Ref, Note |
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Galactic longitude (°) | 70.8963Ref | Proper motion in α (mas/yr) | -2.96±0.03Ref | ||
Galactic latitude (°) | 4.7420Ref | Proper motion in δ (mas/yr) | -2.88±0.03Ref |
X-Ray | NoRef | IR type | SRef | Radio | YesRef |
X-Ray type | - | J (mag) | 5.76Ref | Flickering | NoRef |
GALEX FUV (mag) | - | H (mag) | 4.76Ref | Outbursts | YesRef |
GALEX NUV (mag) | - | K (mag) | 4.41Ref | Outburst type | Z AndRef |
IUE | YesRef | WISE W1 (mag) | 4.29Ref | Jets | - |
FUSE | NoRef | WISE W2 (mag) | 4.07Ref | Resolved nebula | NoRef |
U (mag) | - | WISE W3 (mag) | 4.01Ref | IPmax (eV) | 99.0Ref, 109.3 (UV)Ref |
B (mag) | 12.13Ref | WISE W4 (mag) | 3.57Ref | [O III] lines | YesRef |
V (mag) | 10.93Ref | IRAS 12μm (Jy) | 0.93Ref | He II lines | YesRef |
R (mag) | - | IRAS 25μm (Jy) | 0.33Ref | [Fe VII] lines | YesRef |
I (mag) | - | IRAS 60μm (Jy) | 0.45Ref | O VI lines | NoRef |
BP (mag) | 10.87Ref | IRAS 100μm (Jy) | 5.97Ref | ||
G (mag) | 9.20Ref | AKARI S09 (Jy) | 1.22Ref | ||
RP (mag) | 7.90Ref | AKARI S18 (Jy) | 0.41Ref |
Orbital period (days) | 855.6Ref, 853.8±2.9Ref | γ velocity (km/h) | 18.3±0.4Ref, 14.96±0.23Ref, 9.17±2.48Ref |
Size of giant’s orbit (AU) | 0.544Ref, 0.523Ref |
Eccentricity | 0.15±0.08Ref, 0.109±0.048Ref | RV of giant (km/h) | 7±0.5Ref, 6.7±0.3Ref | Separation (AU) | - |
Inclination (°) | >86Ref, 73±6Ref | Inferior conj. of giant (JD) | 2445323.8,2450426.4 | Mass function | 0.029Ref, 0.0262Ref |
Eclipses | YesRef | Mass ratio | 3Ref, 3Ref | ||
Orbital ephemeris | Min (B) = 2442687.1 + 855.6 x ERef |
Spectral type | M4 IIIRef, M4.9 IIIRef, M5 IIIRef, M5.5 IIIRef |
Mass (M⊙) | 2.4±0.6Ref, 1.5Ref, 1.3±0.3Ref |
Pulsation | - |
Eff. temperature (K) | 3300Ref | Radius (R⊙) | 250±30Ref, 240±20Ref, 180Ref |
Type | - |
IR type | SRef | Luminosity (L⊙) | 4200-7000Ref, 4500Ref, 3400Ref |
Pulsation period (days) | - |
Metallicity [Fe/H] | -0.1±0.07Ref | Pulsation ephemeris | - |
Type/Spectral type | WDRef | Mass (M⊙) | 0.5Ref, 0.43±0.04Ref | Spin period (min) | 66.6?Ref |
Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | 0.06-0.08Ref, 0.006Ref | Accretion disk | - |
Eff. temperature (K) | 130000Ref, 156000±5000Ref, 90000-155000Ref, 125000Ref, 115000Ref, 115000Ref |
Luminosity (L⊙) | 760-2200Ref, 560Ref, 1700Ref |
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Lower limit (K) | - | ||||
Upper limit (K) | - |
Swings & Struve (1940) indicated a possible detection of the coronal [Fe X] line.