AS 288
LIKELY
MILKY WAY
Constellation
Sagittarius |
Equatorial coordinates
α = 18 12 47.981
δ = -28 19 59.807 |
Galactic coordinates
l = 3.4920°
b = -4.8740° |
Suspected |
1978Ref |
Confirmed |
- |
Symbiotic IR type |
D?Ref |
Hot component type |
shell-burning?Ref |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
AS 288 (Susp.) |
Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
AS 288 (Susp.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
Right ascension (°) |
273.1999Ref |
Parallax (mas) |
0.126±0.028Ref |
Reddening E(B-V) (mag) |
0.42±0.02Ref, Note |
Declination (°) |
-28.3333Ref |
Distance (kpc) |
6.34Ref, Note, 6.29Ref, Note |
|
|
Galactic longitude (°) |
3.4920Ref |
Proper motion in α (mas/yr) |
-4.03±0.03Ref |
|
|
Galactic latitude (°) |
-4.8740Ref |
Proper motion in δ (mas/yr) |
-4.07±0.02Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
D?Ref |
Radio |
NoRef, YesRef |
X-Ray type |
- |
J (mag) |
11.47Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
9.75Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
8.31Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
6.76Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
5.82Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
4.06Ref |
IPmax (eV) |
54.4Ref |
B (mag) |
12.00Ref |
WISE W4 (mag) |
2.73Ref |
[O III] lines |
- |
V (mag) |
14.20Ref |
IRAS 12μm (Jy) |
1.24Ref |
He II lines |
YesRef |
R (mag) |
- |
IRAS 25μm (Jy) |
1.10Ref |
[Fe VII] lines |
NoRef |
I (mag) |
- |
IRAS 60μm (Jy) |
4.33Ref |
O VI lines |
NoRef |
BP (mag) |
14.03Ref |
IRAS 100μm (Jy) |
49.30Ref |
|
|
G (mag) |
13.62Ref |
AKARI S09 (Jy) |
0.80Ref |
|
|
RP (mag) |
12.85Ref |
AKARI S18 (Jy) |
0.70Ref |
|
|
Orbit
Orbital period (days) |
1250Ref |
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 |
- |
Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
- |
IR type |
D?Ref |
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-burning?Ref |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Mentioned as a symbiotic star in Wright & Allen (1978). List as a suspected symbiotic binary in Belczyński et al. (2000). Its spectrum exhibits emission-lines with ionization potential up to 54.4 eV, but no late-type giant. In the IR diagram, it is situated among D-type symbiotic stars. The symbiotic nature is further supported by the analysis of IR data by Akras et al. (2019).
References
- Akras, S., Leal-Ferreira, M. L., Guzman-Ramirez, L. et al., 2019, MNRAS, 483, 4, 5077, 2019MNRAS.483.5077A
- Belczyński, K., Mikołajewska, J., Munari, U. et al., 2000, A&AS, 146, 407, 2000A&AS..146..407B
- Wright, A. E., Allen, D. A., 1978, MNRAS, 184, 893, 1978MNRAS.184..893W
Last updated: August 20, 2021