January 13, 2024
New objects added
January 17, 2023
Gaia DR3 candidates added
January 15, 2023
Utilities and search added
January 4, 2023
New version fully released
November 7, 2022
New version testing started
Jan 28, 2019
First public release
All symbiotics
Galactic symbiotics
Extragalactic symbiotics
Version from February 3, 2024
POSSIBLE
MILKY WAY
|
| DT Psc | IRAS 01113+2815 | GSC2.4.2 NBLP000284 | AAVSO 000-BBC-560 |
| SIMBAD V* DT Psc | Pan-STARRS - | SAO 74576 | VSX 26538 |
| GAIA DR3 308866701872125568 | SkyMapper - | WRAY - | GCVS DT Psc |
| 2MASS J01140490+2831464 | HIP 5772 | Hen - | BD +27 196 |
| WISE J011404.96+283146.0 | TYC 1753-2053-1 | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 18.5207Ref | Parallax (mas) | 3.347±0.103Ref | Reddening E(B-V) (mag) | 0.05±0.0Ref, Note |
| Declination (°) | 28.5293Ref | Distance (kpc) | 0.30Ref, Note, 0.30Ref, Note | ||
| Galactic longitude (°) | 128.9382Ref | Proper motion in α (mas/yr) | 61.02±0.10Ref | ||
| Galactic latitude (°) | -34.0782Ref | Proper motion in δ (mas/yr) | -53.01±0.08Ref |
| X-Ray | YesRef | IR type | S?Ref | Radio | NoRef |
| X-Ray type | - | J (mag) | 2.73Ref | Flickering | - |
| GALEX FUV (mag) | 18.93Ref | H (mag) | 1.86Ref | Outbursts | - |
| GALEX NUV (mag) | 16.80Ref | K (mag) | 1.64Ref | Outburst type | - |
| IUE | YesRef | WISE W1 (mag) | -0.70Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 0.17Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 1.47Ref | IPmax (eV) | - |
| B (mag) | 8.36Ref | WISE W4 (mag) | 1.36Ref | [O III] lines | - |
| V (mag) | 7.47Ref | IRAS 12μm (Jy) | 11.50Ref | He II lines | - |
| R (mag) | - | IRAS 25μm (Jy) | 3.01Ref | [Fe VII] lines | - |
| I (mag) | - | IRAS 60μm (Jy) | 0.61Ref | O VI lines | - |
| BP (mag) | 6.64Ref | IRAS 100μm (Jy) | 1.00Ref | ||
| G (mag) | 5.36Ref | AKARI S09 (Jy) | 15.07Ref | ||
| RP (mag) | 4.24Ref | AKARI S18 (Jy) | 3.45Ref |
| Orbital period (days) | 4596±7Ref | γ velocity (km/h) | 1.67±0.02Ref, 5.95±0.24Ref | Size of giant’s orbit (AU) | - |
| Eccentricity | 0.18±0.01Ref | RV of giant (km/h) | 5.38±0.03Ref | Separation (AU) | - |
| Inclination (°) | - | Inferior conj. of giant (JD) | - | Mass function | 0.07Ref |
| Eclipses | - | Mass ratio | - | ||
| Orbital ephemeris | T0 = 2444703±20 + 4596±7 x ERef |
| Spectral type | S3/2Ref | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | 3548Ref, 3600Ref | Radius (R⊙) | - | Type | - |
| IR type | S?Ref | Luminosity (L⊙) | - | Pulsation period (days) | - |
| Metallicity [Fe/H] | 0.02Ref | Pulsation ephemeris | - |
| Type/Spectral type | - | 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) | - |
The star has been mentioned to display mild symbiotic activity in the literature (Smith et al., 1997; Jorissen et al., 2012, 2019). The IUE spectrum did not reveal a prominent contribution from the hot component according to Ake et al. (1988). In addition, X-ray emission from the star was detected by Jorissen et al. (1996). The orbital period of the star was determined to be 4596 days by Jorissen et al. (2019).