V917 Sco
CONFIRMED
MILKY WAY
Constellation
Scorpius |
Equatorial coordinates
α = 17 48 04.274
δ = -36 08 17.418 |
Galactic coordinates
l = 354.0997°
b = -4.1693° |
Suspected |
1978Ref |
Confirmed |
1978Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
YesRef - SyN?Ref |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
Hen 1481 (Conf.) |
Belzcyński et al. (2001) |
V917 Sco (Conf.) |
Gaposchkin (1957) |
- |
Kenyon (1986) |
V917 Sco (Conf.) |
Akras et al. (2019) |
V917 Sco (Conf.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
V917 Sco (Conf.) |
Position
Right ascension (°) |
267.0178Ref |
Parallax (mas) |
0.084±0.032Ref |
Reddening E(B-V) (mag) |
0.58±0.02Ref, Note |
Declination (°) |
-36.1382Ref |
Distance (kpc) |
6.79Ref, Note, 6.03Ref, Note |
|
|
Galactic longitude (°) |
354.0997Ref |
Proper motion in α (mas/yr) |
-4.85±0.04Ref |
|
|
Galactic latitude (°) |
-4.1693Ref |
Proper motion in δ (mas/yr) |
-5.58±0.02Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
SRef |
Radio |
NoRef |
X-Ray type |
- |
J (mag) |
9.42Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
8.30Ref |
Outbursts |
YesRef |
GALEX NUV (mag) |
- |
K (mag) |
7.85Ref |
Outburst type |
SyN?Ref |
IUE |
NoRef |
WISE W1 (mag) |
7.63Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
7.74Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
7.36Ref |
IPmax (eV) |
114Ref |
B (mag) |
13.90Ref |
WISE W4 (mag) |
6.98Ref |
[O III] lines |
YesRef |
V (mag) |
15.00Ref |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
R (mag) |
- |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
YesRef |
I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
YesRef |
BP (mag) |
15.59Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
13.60Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
12.19Ref |
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 |
M7Ref |
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) |
- |
Luminosity (L⊙) |
- |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Detected in a long-lasting outburst, the light curve is presented in Chaisson (1977).
References
- Allen, D. A., 1978, MNRAS, 184, 601, 1978MNRAS.184..601A
- Chaisson, L. J., 1977, PASP, 89, 901, 1977PASP...89..901C
Last updated: May 11, 2020