LIN 358
CONFIRMED
SMC
Constellation
Tucana |
Equatorial coordinates
α = 00 59 12.255
δ = -75 05 17.633 |
Galactic coordinates
l = 302.2594°
b = -42.0299° |
Suspected |
1983Ref |
Confirmed |
1983Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
SMC Ln 358 (Conf.) |
Belzcyński et al. (2001) |
LIN 358 (Conf.) |
Gaposchkin (1957) |
- |
Kenyon (1986) |
SMC Ln 358 (Conf.) |
Akras et al. (2019) |
LIN 358 (Conf.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
Lin 358 (Conf.) |
Position
Right ascension (°) |
14.8011Ref |
Parallax (mas) |
-0.039±0.017Ref |
Reddening E(B-V) (mag) |
0.04±0.0Ref, Note |
Declination (°) |
-75.0882Ref |
Distance (kpc) |
62.1±1.9Ref 31.10Ref, Note, 22.22Ref, Note |
|
|
Galactic longitude (°) |
302.2594Ref |
Proper motion in α (mas/yr) |
0.83±0.02Ref |
|
|
Galactic latitude (°) |
-42.0299Ref |
Proper motion in δ (mas/yr) |
-1.08±0.02Ref |
|
|
Observations
X-Ray |
YesRef |
IR type |
SRef |
Radio |
- |
X-Ray type |
αRef |
J (mag) |
12.50Ref |
Flickering |
- |
GALEX FUV (mag) |
18.52Ref |
H (mag) |
11.65Ref |
Outbursts |
- |
GALEX NUV (mag) |
18.74Ref |
K (mag) |
11.46Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
11.29Ref |
Jets |
- |
FUSE |
YesRef |
WISE W2 (mag) |
11.29Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
10.86Ref |
IPmax (eV) |
114Ref |
B (mag) |
16.82Ref |
WISE W4 (mag) |
8.90Ref |
[O III] lines |
NoRef |
V (mag) |
15.34Ref |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
R (mag) |
14.90Ref |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
NoRef |
I (mag) |
13.77Ref |
IRAS 60μm (Jy) |
- |
O VI lines |
YesRef |
BP (mag) |
15.58Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
14.71Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
13.77Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
~1060?Ref |
γ velocity (km/h) |
155.61±5.09Ref |
Size of giant’s orbit (AU) |
- |
Eccentricity |
- |
RV of giant (km/h) |
- |
Separation (AU) |
3.7Ref |
Inclination (°) |
- |
Inferior conj. of giant (JD) |
- |
Mass function |
- |
Eclipses |
- |
|
|
Mass ratio |
4Ref |
Orbital ephemeris |
- |
|
|
|
|
Cool component
Spectral type |
K5 IbRef |
Mass (M⊙) |
5Ref, 2.31±0.79Ref |
Pulsation |
- |
Eff. temperature (K) |
4000±200Ref |
Radius (R⊙) |
178±18Ref |
Type |
- |
IR type |
SRef |
Luminosity (L⊙) |
7300Ref |
Pulsation period (days) |
- |
Metallicity [Fe/H] |
-1±0.1Ref |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
WDRef |
Mass (M⊙) |
>1.18Ref, >0.57Ref |
Spin period (min) |
- |
Shell-burning/Accreting-only |
shell-burningRef |
Radius (R⊙) |
0.089Ref, 0.127Ref |
Accretion disk |
- |
Eff. temperature (K) |
160000Ref, 250000Ref |
Luminosity (L⊙) |
26660±3920Ref |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
The symbiotic star LIN 358 is identified as a super-soft X-ray source.
References
- Akras, S., Guzman-Ramirez, L., Leal-Ferreira, M. L. et al., 2019, ApJS, 240, 2, 21, 2019ApJS..240...21A
- Kuuttila, J., Gilfanov, M., Woods, T. E. et al., 2021, MNRAS, 500, 3, 3763, 2021MNRAS.500.3763K
- Morgan, D. H., 1992, MNRAS, 258, 639, 1992MNRAS.258..639M
- Mürset, U., Wolff, B., Jordan, S., 1997, A&A, 319, 201, 1997A&A...319..201M
- Orio, M., Zezas, A., Munari, U. et al., 2007, ApJ, 661, 2, 1105, 2007ApJ...661.1105O
- Skopal, A., 2015, NewA, 36, 116, 2015NewA...36..116S
- Washington, J. E., Lewis, H. M., Anguiano, B. et al., 2021, ApJ, 918, 1, 19, 2021ApJ...918...19W
Last updated: August 21, 2021