CONFIRMED
MILKY WAY
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RW Hya | IRAS 13315-2507 | GSC2.4.2 S6KH000359 | AAVSO 000-BCW-104 |
SIMBAD V* RW Hya | Pan-STARRS 77542035755084069 | SAO 81760 | VSX 15974 |
GAIA DR3 6191401382471531264 | SkyMapper - | WRAY - | GCVS RW Hya |
2MASS J13341813-2522489 | HIP - | Hen 3-917 | BD - |
WISE J133418.11-252248.6 | TYC 6718-1146-1 | ESO - | HD 117970 |
Bidelman (1954) | RW Hya (Conf.) | Allen (1984) | RW Hya (Conf.) | Belzcyński et al. (2001) | RW Hya (Conf.) |
Gaposchkin (1957) | RW Hya (Conf.) | Kenyon (1986) | RW Hya (Conf.) | Akras et al. (2019) | RW Hya (Conf.) |
Boyarchuk (1969) | RW Hya (Conf.) | Vaidis (1988, 1991) | RW Hya (Conf.) |
Right ascension (°) | 203.5754Ref | Parallax (mas) | 0.648±0.035Ref | Reddening E(B-V) (mag) | 0.06±0.0Ref, Note |
Declination (°) | -25.3802Ref | Distance (kpc) | 1.3Ref, 0.6Ref, 1.0Ref, 0.67Ref, 0.82±0.112Ref 1.48Ref, Note, 1.49Ref, Note |
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Galactic longitude (°) | 314.9926Ref | Proper motion in α (mas/yr) | -17.83±0.03Ref | ||
Galactic latitude (°) | 36.4857Ref | Proper motion in δ (mas/yr) | 13.21±0.02Ref |
X-Ray | NoRef | IR type | SRef | Radio | YesRef |
X-Ray type | - | J (mag) | 5.73Ref | Flickering | NoRef |
GALEX FUV (mag) | - | H (mag) | 4.92Ref | Outbursts | - |
GALEX NUV (mag) | 13.64Ref | K (mag) | 4.61Ref | Outburst type | - |
IUE | YesRef | WISE W1 (mag) | 4.57Ref | Jets | - |
FUSE | YesRef | WISE W2 (mag) | 4.34Ref | Resolved nebula | NoRef |
U (mag) | - | WISE W3 (mag) | 4.28Ref | IPmax (eV) | 54.4Ref, 77.5 (UV)Ref |
B (mag) | 10.31Ref | WISE W4 (mag) | 3.73Ref | [O III] lines | YesRef |
V (mag) | 10.00Ref | IRAS 12μm (Jy) | 0.88Ref | He II lines | YesRef |
R (mag) | - | IRAS 25μm (Jy) | 0.45Ref | [Fe VII] lines | NoRef |
I (mag) | - | IRAS 60μm (Jy) | 0.40Ref | O VI lines | NoRef |
BP (mag) | 9.04Ref | IRAS 100μm (Jy) | 1.06Ref | ||
G (mag) | 8.12Ref | AKARI S09 (Jy) | 0.94Ref | ||
RP (mag) | 7.14Ref | AKARI S18 (Jy) | 0.29Ref |
Orbital period (days) | 372.45±0.3Ref, 370.2±0.9Ref, 370.4±0.8Ref |
γ velocity (km/h) | 12.4±0.3Ref, 12.9±0.4Ref | Size of giant’s orbit (AU) | 0.3Ref |
Eccentricity | 0±-Ref | RV of giant (km/h) | 8.8±0.5Ref, 8.8±0.4Ref | Separation (AU) | 1.29±0.08Ref |
Inclination (°) | 90Ref | Inferior conj. of giant (JD) | 2445071.6 | Mass function | 0.019Ref, 0.026Ref, 0.026Ref |
Eclipses | YesRef | Mass ratio | 3.3Ref | ||
Orbital ephemeris | Max (pg) = 2421519.2±4.2 + 372.45±0.3 x ERef |
Spectral type | M2 IIIRef, M0 IIIRef, M1.1 IIIRef, M2 IIIRef |
Mass (M⊙) | 0.5-2Ref, 1.6±0.3Ref, 3.4Ref |
Pulsation | - |
Eff. temperature (K) | 3770±50Ref, 3800Ref, 3655±80Ref, 3900Ref |
Radius (R⊙) | 83Ref, 70Ref, 58.5±8Ref, 145Ref |
Type | - |
IR type | SRef | Luminosity (L⊙) | 602Ref, 1000Ref, 625±200Ref, 650±180Ref |
Pulsation period (days) | - |
Metallicity [Fe/H] | -0.76±0.06Ref, -0.64±0.14Ref, -0.77±0.08Ref |
Pulsation ephemeris | - |
Type/Spectral type | WDRef | Mass (M⊙) | 0.3-0.6Ref, 0.48±0.06Ref | Spin period (min) | - |
Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | 0.12-0.13Ref, 0.10Ref, 0.036±0.01Ref, 0.066Ref |
Accretion disk | - |
Eff. temperature (K) | 50000-100000Ref, 70000-90000Ref, 75000Ref, 110000±30000Ref, 160000±10000Ref |
Luminosity (L⊙) | 100-1250Ref, 200Ref, 290Ref, 2000-3300Ref |
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Lower limit (K) | - | ||||
Upper limit (K) | - |
Discovered by Merrill & Humason (1932), this star exhibited an "anomalous combination in a single spectrum of features which ordinarily occur near opposite ends of the sequence of stellar temperatures." Subsequent observations by Merrill & Burwell (1933) revealed the presence of TiO bands and a strong He II line. No outburst of this star has been recorded to date (Kenyon & Mikołajewska, 1995). Further investigations by Sion et al. (2002) reported possible outflows associated with the white dwarf component.