RT Car
SUSPECTED
MILKY WAY
Constellation
Carina |
Equatorial coordinates
α = 10 44 47.133
δ = -59 24 48.077 |
Galactic coordinates
l = 287.4396°
b = -0.4060° |
Suspected |
1977Ref |
Confirmed |
- |
Symbiotic IR type |
S/D?Ref |
Hot component type |
accreting-only?Ref |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
- |
Gaposchkin (1957) |
- |
Kenyon (1986) |
RT Car (Susp.) |
Akras et al. (2019) |
- |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
RT Car (Conf.) |
Position
Right ascension (°) |
161.1964Ref |
Parallax (mas) |
0.438±0.027Ref |
Reddening E(B-V) (mag) |
7.09±1.54Ref, Note |
Declination (°) |
-59.4134Ref |
Distance (kpc) |
2.13Ref, Note, 2.14Ref, Note |
|
|
Galactic longitude (°) |
287.4396Ref |
Proper motion in α (mas/yr) |
-7.43±0.03Ref |
|
|
Galactic latitude (°) |
-0.4060Ref |
Proper motion in δ (mas/yr) |
2.85±0.03Ref |
|
|
Observations
X-Ray |
YesRef |
IR type |
S/D?Ref |
Radio |
NoRef |
X-Ray type |
β/δRef |
J (mag) |
2.97Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
1.95Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
1.50Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
-0.77Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
-0.22Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
-1.44Ref |
IPmax (eV) |
No linesRef |
B (mag) |
11.82Ref |
WISE W4 (mag) |
-2.05Ref |
[O III] lines |
NoRef |
V (mag) |
9.54Ref |
IRAS 12μm (Jy) |
85.50Ref |
He II lines |
NoRef |
R (mag) |
- |
IRAS 25μm (Jy) |
98.70Ref |
[Fe VII] lines |
NoRef |
I (mag) |
- |
IRAS 60μm (Jy) |
372.00Ref |
O VI lines |
NoRef |
BP (mag) |
8.93Ref |
IRAS 100μm (Jy) |
873.00Ref |
|
|
G (mag) |
6.90Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
5.61Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
- |
γ velocity (km/h) |
-21.95±0.58Ref |
Size of giant’s orbit (AU) |
- |
Eccentricity |
- |
RV of giant (km/h) |
- |
Separation (AU) |
- |
Inclination (°) |
- |
Inferior conj. of giant (JD) |
- |
Mass function |
- |
Eclipses |
- |
|
|
Mass ratio |
- |
Orbital ephemeris |
- |
|
|
|
|
Cool component
Spectral type |
M2 IRef |
Mass (M⊙) |
- |
Pulsation |
YesRef |
Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
- |
IR type |
S/D?Ref |
Luminosity (L⊙) |
- |
Pulsation period (days) |
163.3Ref |
Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
OB?Ref |
Mass (M⊙) |
- |
Spin period (min) |
- |
Shell-burning/Accreting-only |
accreting-only?Ref |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
The star was included in the list of symbiotic binaries by Payne-Gaposchkin (1977). However, Schulte-Ladbeck (1988) did not detect any emission lines in the spectra, and it is unclear on which data the original suggestion is based.
References
- Payne-Gaposchkin, C. H., 1977, AJ, 82, 665, 1977AJ.....82..665P
- Schulte-Ladbeck, R. E., 1988, A&A, 189, 97, 1988A&A...189...97S
Last updated: June 1, 2021