AS 281
CONFIRMED
MILKY WAY
Constellation
Sagittarius |
Equatorial coordinates
α = 18 10 43.858
δ = -27 57 50.145 |
Galactic coordinates
l = 3.6002°
b = -4.2972° |
Suspected |
1969Ref |
Confirmed |
1984Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
AS 281 (Conf.) |
Belzcyński et al. (2001) |
AS 281 (Conf.) |
Gaposchkin (1957) |
- |
Kenyon (1986) |
AS 281 (Conf.) |
Akras et al. (2019) |
AS 281 (Conf.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
Ap1-10 (Conf.) |
Position
Right ascension (°) |
272.6827Ref |
Parallax (mas) |
0.209±0.041Ref |
Reddening E(B-V) (mag) |
0.48±0.03Ref, Note |
Declination (°) |
-27.9639Ref |
Distance (kpc) |
7Ref, 4.5Ref 5.02Ref, Note, 4.38Ref, Note |
|
|
Galactic longitude (°) |
3.6002Ref |
Proper motion in α (mas/yr) |
-3.47±0.04Ref |
|
|
Galactic latitude (°) |
-4.2972Ref |
Proper motion in δ (mas/yr) |
-2.53±0.03Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
SRef |
Radio |
YesRef |
X-Ray type |
- |
J (mag) |
8.30Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
7.28Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
6.92Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
6.69Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
6.80Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
6.50Ref |
IPmax (eV) |
114Ref |
B (mag) |
12.00Ref |
WISE W4 (mag) |
6.09Ref |
[O III] lines |
NoRef |
V (mag) |
13.60Ref |
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) |
14.00Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
12.13Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
10.76Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
533±30Ref |
γ velocity (km/h) |
-137.23±1.01Ref |
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 (B) = 2449021 + 533±30 x ERef |
|
|
|
|
Cool component
Spectral type |
M5.5 IIIRef, M5 IIIRef, M3 IIIRef, M6 IIIRef |
Mass (M⊙) |
- |
Pulsation |
YesRef |
Eff. temperature (K) |
3430Ref, 3300Ref |
Radius (R⊙) |
- |
Type |
SRRef |
IR type |
SRef |
Luminosity (L⊙) |
- |
Pulsation period (days) |
65±1Ref |
Metallicity [Fe/H] |
-0.36±0.08Ref |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
WDRef |
Mass (M⊙) |
- |
Spin period (min) |
31.4Ref |
Shell-burning/Accreting-only |
shell-burningRef |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
2800Ref |
|
|
Lower limit (K) |
114000Ref |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Herbig (1969) reported a strong continuous spectrum with intense Hβ and He II. Stenholm & Acker (1987) detected [Fe VII] and O VI lines. Toma et al. (2016) identified variability with a period of 31.4 minutes and an amplitude of 0.008 mag. It might represent a rotational period of a magnetic white dwarf, similar to Z And.
References
- Allen, D. A., 1980, MNRAS, 192, 521, 1980MNRAS.192..521A
- Allen, D. A., 1984, PASA, 5, 3, 369, 1984PASA....5..369A
- Gałan, C., Mikołajewska, J., Hinkle, K. H. et al., 2017, MNRAS, 466, 2, 2194, 2017MNRAS.466.2194G
- Gromadzki, M., Mikołajewska, J., Soszyński, I., 2013, AcA, 63, 4, 405, 2013AcA....63..405G
- Herbig, G. H., 1969, PNAS, 63, 4, 1045, 1969PNAS...63.1045H
- 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
- Stenholm, B., Acker, A., 1987, A&AS, 68, 51, 1987A&AS...68...51S
- Toma, R., Ramsay, G., Macfarlane, S. et al., 2016, MNRAS, 463, 1, 1099, 2016MNRAS.463.1099T
Last updated: April 18, 2022