ASASSN-V J173832.43-492840.2
SUSPECTED
MILKY WAY
Constellation
Ara |
Equatorial coordinates
α = 17 38 32.412
δ = -49 28 40.233 |
Galactic coordinates
l = 341.6735°
b = -9.5421° |
Suspected |
2018Ref |
Confirmed |
- |
Symbiotic IR type |
S?Ref |
Hot component type |
accreting-only?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 (°) |
264.6350Ref |
Parallax (mas) |
-0.019±0.076Ref |
Reddening E(B-V) (mag) |
0.15±0.01Ref, Note |
Declination (°) |
-49.4778Ref |
Distance (kpc) |
7.94Ref, Note, 6.92Ref, Note |
|
|
Galactic longitude (°) |
341.6735Ref |
Proper motion in α (mas/yr) |
-3.26±0.08Ref |
|
|
Galactic latitude (°) |
-9.5421Ref |
Proper motion in δ (mas/yr) |
-7.67±0.06Ref |
|
|
Observations
X-Ray |
- |
IR type |
S?Ref |
Radio |
- |
X-Ray type |
- |
J (mag) |
8.04Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
7.12Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
6.61Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
6.86Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
6.42Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
5.58Ref |
IPmax (eV) |
- |
B (mag) |
15.62Ref |
WISE W4 (mag) |
4.66Ref |
[O III] lines |
- |
V (mag) |
13.90Ref |
IRAS 12μm (Jy) |
- |
He II lines |
- |
R (mag) |
- |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
- |
I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
- |
BP (mag) |
17.92Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
14.09Ref |
AKARI S09 (Jy) |
0.37Ref |
|
|
RP (mag) |
12.44Ref |
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 |
YesRef |
Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
MiraRef |
IR type |
S?Ref |
Luminosity (L⊙) |
- |
Pulsation period (days) |
366.2Ref |
Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
- |
Mass (M⊙) |
- |
Spin period (min) |
- |
Shell-burning/Accreting-only |
accreting-only?Ref |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Symbiotic candidate selected for AAVSO observing campaing (AAVSO Alert Notice 650) by Adrian B. Lucy (Columbia University). It is also classified as a long-period variable candidate by Mowlavi et al. (2018).
References
- Mowlavi, N., Lecoeur-Taïbi, I., Lebzelter, T. et al., 2018, A&A, 618, A58, 2018A&A...618A..58M
Last updated: August 23, 2021