AS 327
CONFIRMED
MILKY WAY
Constellation
Sagittarius |
Equatorial coordinates
α = 18 53 16.658
δ = -24 22 58.845 |
Galactic coordinates
l = 11.1428°
b = -11.2303° |
Suspected |
1967Ref |
Confirmed |
1969Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
AS 327 (Conf.) |
Belzcyński et al. (2001) |
AS 327 (Conf.) |
Gaposchkin (1957) |
- |
Kenyon (1986) |
AS 327 (Conf.) |
Akras et al. (2019) |
AS 327 (Conf.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
MHA 208-67 (Conf.) |
Position
Right ascension (°) |
283.3194Ref |
Parallax (mas) |
0.149±0.023Ref |
Reddening E(B-V) (mag) |
0.41±0.01Ref, Note |
Declination (°) |
-24.3830Ref |
Distance (kpc) |
3Ref 5.88Ref, Note, 5.47Ref, Note |
|
|
Galactic longitude (°) |
11.1428Ref |
Proper motion in α (mas/yr) |
-4.21±0.03Ref |
|
|
Galactic latitude (°) |
-11.2303Ref |
Proper motion in δ (mas/yr) |
-2.73±0.02Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
SRef |
Radio |
YesRef |
X-Ray type |
- |
J (mag) |
8.83Ref |
Flickering |
- |
GALEX FUV (mag) |
17.19Ref |
H (mag) |
7.87Ref |
Outbursts |
- |
GALEX NUV (mag) |
16.70Ref |
K (mag) |
7.55Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
7.45Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
7.43Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
7.02Ref |
IPmax (eV) |
114Ref |
B (mag) |
14.74Ref |
WISE W4 (mag) |
6.24Ref |
[O III] lines |
NoRef |
V (mag) |
13.09Ref |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
R (mag) |
- |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
NoRef |
I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
YesRef |
BP (mag) |
13.07Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
11.81Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
10.65Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
823±55Ref |
γ velocity (km/h) |
8.81±2.70Ref |
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 (V) = 2451954 + 823±55 x ERef |
|
|
|
|
Cool component
Spectral type |
M4 IIIRef, M0 IIIRef, M2 IIIRef |
Mass (M⊙) |
- |
Pulsation |
YesRef |
Eff. temperature (K) |
3560Ref |
Radius (R⊙) |
- |
Type |
SRRef |
IR type |
SRef |
Luminosity (L⊙) |
- |
Pulsation period (days) |
83±1Ref |
Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
WDRef |
Mass (M⊙) |
- |
Spin period (min) |
- |
Shell-burning/Accreting-only |
shell-burningRef |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
2700Ref |
|
|
Lower limit (K) |
114000Ref |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Herbig (1969) reported that the object has an early M-type spectrum with bright H and He II lines.
References
- Gromadzki, M., Mikołajewska, J., Soszyński, I., 2013, AcA, 63, 4, 405, 2013AcA....63..405G
- Henize, K. G., 1967, ApJS, 14, 125, 1967ApJS...14..125H
- Herbig, G. H., 1969, PNAS, 63, 4, 1045, 1969PNAS...63.1045H
- Luna, G. J. M., Sokoloski, J. L., Mukai, K. et al., 2013, A&A, 559, A6, 2013A&A...559A...6L
- 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
- Mürset, U., Schmid, H. M., 1999, A&AS, 137, 473, 1999A&AS..137..473M
- Swings, J. P., Allen, D. A., 1972, PASP, 84, 500, 523, 1972PASP...84..523S
Last updated: April 18, 2022