SS73 122
CONFIRMED
MILKY WAY
Constellation
Sagittarius |
Equatorial coordinates
α = 18 04 41.215
δ = -27 09 12.514 |
Galactic coordinates
l = 3.6625°
b = -2.7328° |
Suspected |
1980Ref |
Confirmed |
1984Ref |
Symbiotic IR type |
DRef, SRef |
Hot component type |
shell-burningRef |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
SS 122 (Conf.) |
Belzcyński et al. (2001) |
SS73 122 (Conf.) |
Gaposchkin (1957) |
- |
Kenyon (1986) |
SS 122 (Conf.) |
Akras et al. (2019) |
SS73 122 (Conf.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
VDS 114 (Conf.) |
Position
Right ascension (°) |
271.1717Ref |
Parallax (mas) |
-0.026±0.055Ref |
Reddening E(B-V) (mag) |
1.1±0.04Ref, Note |
Declination (°) |
-27.1535Ref |
Distance (kpc) |
4.8Ref 9.25Ref, Note, 7.34Ref, Note |
|
|
Galactic longitude (°) |
3.6625Ref |
Proper motion in α (mas/yr) |
-3.89±0.07Ref |
|
|
Galactic latitude (°) |
-2.7328Ref |
Proper motion in δ (mas/yr) |
-5.65±0.05Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
DRef, SRef |
Radio |
YesRef |
X-Ray type |
- |
J (mag) |
8.31Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
7.06Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
6.36Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
5.68Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
5.25Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
4.03Ref |
IPmax (eV) |
114Ref |
B (mag) |
- |
WISE W4 (mag) |
3.04Ref |
[O III] lines |
YesRef |
V (mag) |
15.42Ref |
IRAS 12μm (Jy) |
1.44Ref |
He II lines |
YesRef |
R (mag) |
- |
IRAS 25μm (Jy) |
1.00Ref |
[Fe VII] lines |
YesRef |
I (mag) |
12.63Ref |
IRAS 60μm (Jy) |
13.20Ref |
O VI lines |
YesRef |
BP (mag) |
14.33Ref |
IRAS 100μm (Jy) |
212.00Ref |
|
|
G (mag) |
13.17Ref |
AKARI S09 (Jy) |
1.27Ref |
|
|
RP (mag) |
11.89Ref |
AKARI S18 (Jy) |
0.71Ref |
|
|
Orbit
Orbital period (days) |
2409±10Ref |
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 |
Min (RI) = 2446709 + 2409±10 x ERef |
|
|
|
|
Cool component
Spectral type |
M7.5 IIIRef, M7 IIIRef |
Mass (M⊙) |
- |
Pulsation |
YesRef |
Eff. temperature (K) |
3073Ref |
Radius (R⊙) |
- |
Type |
SRRef |
IR type |
DRef, SRef |
Luminosity (L⊙) |
- |
Pulsation period (days) |
189±4Ref |
Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
WDRef |
Mass (M⊙) |
- |
Spin period (min) |
22.8?Ref |
Shell-burning/Accreting-only |
shell-burningRef |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
12000Ref |
|
|
Lower limit (K) |
114000Ref |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Originally identified as a Be star in Sanduleak & Stephenson (1973), it was later suspected to be a Mira pulsator by Whitelock (1987), although the confirmation of an infrared type D has not been established. In Toma et al. (2016), periodic modulation with a period of 22.8 minutes and an amplitude of 0.006 mag was reported.
References
- Allen, D. A., 1980, MNRAS, 192, 521, 1980MNRAS.192..521A
- Gromadzki, M., Mikołajewska, J., Soszyński, I., 2013, AcA, 63, 4, 405, 2013AcA....63..405G
- Medina Tanco, G. A., Steiner, J. E., 1995, AJ, 109, 1770, 1995AJ....109.1770M
- Mikołajewska, J., Acker, A., Stenholm, B., 1997, A&A, 327, 191, 1997A&A...327..191M
- Sanduleak, N., Stephenson, C. B., 1973, ApJ, 185, 899, 1973ApJ...185..899S
- Toma, R., Ramsay, G., Macfarlane, S. et al., 2016, MNRAS, 463, 1, 1099, 2016MNRAS.463.1099T
- Whitelock, P. A., 1987, PASP, 99, 573, 1987PASP...99..573W
Last updated: April 18, 2022