V353 Aur
POSSIBLE
MILKY WAY
Constellation
Auriga |
Equatorial coordinates
α = 04 42 53.624
δ = +36 06 53.401 |
Galactic coordinates
l = 166.4458°
b = -6.5276° |
Suspected |
2014Ref |
Confirmed |
- |
Symbiotic IR type |
D?Ref |
Hot component type |
shell-burning?Ref |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
- |
Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
- |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
Right ascension (°) |
70.7234Ref |
Parallax (mas) |
- |
Reddening E(B-V) (mag) |
0.63±0.01Ref, Note |
Declination (°) |
36.1148Ref |
Distance (kpc) |
-, Note |
|
|
Galactic longitude (°) |
166.4458Ref |
Proper motion in α (mas/yr) |
- |
|
|
Galactic latitude (°) |
-6.5276Ref |
Proper motion in δ (mas/yr) |
- |
|
|
Observations
X-Ray |
NoRef |
IR type |
D?Ref |
Radio |
YesRef |
X-Ray type |
- |
J (mag) |
13.51Ref |
Flickering |
- |
GALEX FUV (mag) |
21.15Ref |
H (mag) |
11.41Ref |
Outbursts |
- |
GALEX NUV (mag) |
19.95Ref |
K (mag) |
8.81Ref |
Outburst type |
- |
IUE |
YesRef |
WISE W1 (mag) |
5.11Ref |
Jets |
YesRef |
FUSE |
NoRef |
WISE W2 (mag) |
1.57Ref |
Resolved nebula |
YesRef |
U (mag) |
- |
WISE W3 (mag) |
-3.01Ref |
IPmax (eV) |
35.1Ref |
B (mag) |
16.32Ref |
WISE W4 (mag) |
-3.58Ref |
[O III] lines |
YesRef |
V (mag) |
- |
IRAS 12μm (Jy) |
471.00Ref |
He II lines |
NoRef |
R (mag) |
12.59Ref |
IRAS 25μm (Jy) |
1110.00Ref |
[Fe VII] lines |
NoRef |
I (mag) |
- |
IRAS 60μm (Jy) |
1040.00Ref |
O VI lines |
NoRef |
BP (mag) |
17.30Ref |
IRAS 100μm (Jy) |
340.00Ref |
|
|
G (mag) |
18.25Ref |
AKARI S09 (Jy) |
189.30Ref |
|
|
RP (mag) |
15.28Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
- |
γ velocity (km/h) |
- |
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 |
- |
Mass (M⊙) |
- |
Pulsation |
- |
Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
- |
IR type |
D?Ref |
Luminosity (L⊙) |
- |
Pulsation period (days) |
- |
Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
- |
Mass (M⊙) |
- |
Spin period (min) |
- |
Shell-burning/Accreting-only |
shell-burning?Ref |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Possible symbiotic classification was suggested by Balick et al. (2014). The central star is not visible in the optical, but they claim it might be an AGB + WC8-type star. The object exhibits a highly bipolar morphology.
References
- Balick, B., Huarte-Espinosa, M., Frank, A. et al., 2013, ApJ, 772, 1, 20, 2013ApJ...772...20B
- Balick, B., Riera, A., Raga, A. et al., 2014, ApJ, 795, 1, 83, 2014ApJ...795...83B
- Phillips, J. P., Williams, P. G., Mampaso, A. et al., 1992, A&A, 260, 283, 1992A&A...260..283P
Last updated: April 6, 2022