SMC1
CONFIRMED
SMC
Constellation
Hydrus |
Equatorial coordinates
α = 00 29 10.829
δ = -74 57 39.886 |
Galactic coordinates
l = 304.8746°
b = -42.0831° |
Suspected |
1992Ref |
Confirmed |
1992Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
SMC1 (Conf.) |
Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
SMC1 (Conf.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
Right ascension (°) |
7.2951Ref |
Parallax (mas) |
-0.004±0.029Ref |
Reddening E(B-V) (mag) |
0.04±0.0Ref, Note |
Declination (°) |
-74.9611Ref |
Distance (kpc) |
62.1±1.9Ref 13.54Ref, Note, 13.99Ref, Note |
|
|
Galactic longitude (°) |
304.8746Ref |
Proper motion in α (mas/yr) |
0.49±0.04Ref |
|
|
Galactic latitude (°) |
-42.0831Ref |
Proper motion in δ (mas/yr) |
-1.27±0.04Ref |
|
|
Observations
X-Ray |
- |
IR type |
SRef |
Radio |
- |
X-Ray type |
- |
J (mag) |
13.65Ref |
Flickering |
- |
GALEX FUV (mag) |
18.23Ref |
H (mag) |
12.85Ref |
Outbursts |
- |
GALEX NUV (mag) |
19.02Ref |
K (mag) |
12.64Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
12.41Ref |
Jets |
- |
FUSE |
YesRef |
WISE W2 (mag) |
12.43Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
11.88Ref |
IPmax (eV) |
114Ref |
B (mag) |
- |
WISE W4 (mag) |
9.07Ref |
[O III] lines |
NoRef |
V (mag) |
16.20Ref |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
R (mag) |
14.70Ref |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
NoRef |
I (mag) |
13.90Ref |
IRAS 60μm (Jy) |
- |
O VI lines |
YesRef |
BP (mag) |
16.55Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
15.84Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
14.98Ref |
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 |
C3.2Ref |
Mass (M⊙) |
- |
Pulsation |
- |
Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
- |
IR type |
SRef |
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-burningRef |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
130000Ref |
Luminosity (L⊙) |
700Ref |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
The star exhibits a rich hydrogen-helium emission-line spectrum superimposed on a carbon star continuum.
References
- Akras, S., Guzman-Ramirez, L., Leal-Ferreira, M. L. et al., 2019, ApJS, 240, 2, 21, 2019ApJS..240...21A
- Morgan, D. H., 1992, MNRAS, 258, 639, 1992MNRAS.258..639M
- Mürset, U., Schild, H., Vogel, M., 1996, A&A, 307, 516, 1996A&A...307..516M
- Mürset, U., Schmid, H. M., 1999, A&AS, 137, 473, 1999A&AS..137..473M
- Mürset, U., Wolff, B., Jordan, S., 1997, A&A, 319, 201, 1997A&A...319..201M
- Phillips, J. P., 2007, MNRAS, 376, 3, 1120, 2007MNRAS.376.1120P
Last updated: May 2, 2019