CONFIRMED
MILKY WAY
|
| CL Sco | IRAS - | GSC2.4.2 S8ET000688 | AAVSO 000-BBY-156 |
| SIMBAD V* CL Sco | Pan-STARRS 71252537165754216 | SAO - | VSX 32928 |
| GAIA DR3 6027978628476711808 | SkyMapper 165451.96-303718.2 | WRAY 15-1564 | GCVS CL Sco |
| 2MASS J16545198-3037181 | HIP - | Hen 3-1286 | BD - |
| WISE J165451.97-303718.2 | TYC - | ESO - | HD - |
| Bidelman (1954) | CL Sco (Conf.) | Allen (1984) | CL Sco (Conf.) | Belzcyński et al. (2001) | CL Sco (Conf.) |
| Gaposchkin (1957) | CL Sco (Conf.) | Kenyon (1986) | CL Sco (Conf.) | Akras et al. (2019) | CL Sco (Conf.) |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | CL Sco (Conf.) |
| Right ascension (°) | 253.7165Ref | Parallax (mas) | 0.042±0.027Ref | Reddening E(B-V) (mag) | 0.28±0.01Ref, Note |
| Declination (°) | -30.6217Ref | Distance (kpc) | 2.3Ref 11.02Ref, Note, 10.71Ref, Note |
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| Galactic longitude (°) | 352.3224Ref | Proper motion in α (mas/yr) | -3.03±0.03Ref | ||
| Galactic latitude (°) | 8.0890Ref | Proper motion in δ (mas/yr) | -0.27±0.02Ref |
| X-Ray | NoRef | IR type | SRef | Radio | YesRef |
| X-Ray type | - | J (mag) | 8.99Ref | Flickering | Yes?Ref |
| GALEX FUV (mag) | - | H (mag) | 8.14Ref | Outbursts | YesRef |
| GALEX NUV (mag) | - | K (mag) | 7.74Ref | Outburst type | Z AndRef |
| IUE | YesRef | WISE W1 (mag) | 7.51Ref | Jets | YesRef |
| FUSE | NoRef | WISE W2 (mag) | 7.41Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 6.86Ref | IPmax (eV) | 54.9Ref |
| B (mag) | 12.59Ref | WISE W4 (mag) | 6.25Ref | [O III] lines | YesRef |
| V (mag) | 11.99Ref | IRAS 12μm (Jy) | - | He II lines | YesRef |
| R (mag) | 12.24Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | NoRef |
| BP (mag) | 12.90Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 11.98Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 10.89Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | 624.7±1.5Ref | γ velocity (km/h) | -35.87±0.35Ref | Size of giant’s orbit (AU) | 0.3937Ref |
| Eccentricity | 0Ref | RV of giant (km/h) | 6.86±0.52Ref | Separation (AU) | - |
| Inclination (°) | - | Inferior conj. of giant (JD) | 2452174.2 | Mass function | 0.0209Ref |
| Eclipses | NoRef | Mass ratio | - | ||
| Orbital ephemeris | Min (pg) = 2427020±21 + 624.7±1.5 x ERef |
| Spectral type | K5 IIIRef, M2 IIIRef, M5 IIIRef |
Mass (M⊙) | 1.5Ref | Pulsation | - |
| Eff. temperature (K) | 3720Ref, 3400Ref | Radius (R⊙) | 75-114Ref | Type | - |
| IR type | SRef | Luminosity (L⊙) | 755Ref | Pulsation period (days) | - |
| Metallicity [Fe/H] | -0.29±0.13Ref | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | 0.035Ref | Accretion disk | - |
| Eff. temperature (K) | 75000-90000Ref | Luminosity (L⊙) | 280Ref, 100Ref | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | 98000Ref |
Swope (1941) noted the variability of the star (outbursts). The star was previously classified as a possible U Geminorum star and SS Cygni-like star. Subsequently, Elvey & Babcock (1943) reported a continuous spectrum with strong Balmer emission lines, He I, He II, and [O III] lines.