PN K4-54
SUSPECTED
MILKY WAY
Constellation
Cygnus |
Equatorial coordinates
α = 20 42 53.279
δ = +45 56 31.041 |
Galactic coordinates
l = 84.9635°
b = 2.2035° |
Suspected |
1974Ref |
Confirmed |
- |
Symbiotic IR type |
S?Ref |
Hot component type |
- |
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 (°) |
310.7220Ref |
Parallax (mas) |
0.129±0.036Ref |
Reddening E(B-V) (mag) |
2.48±0.07Ref, Note |
Declination (°) |
45.9420Ref |
Distance (kpc) |
5.10Ref, Note, 4.63Ref, Note |
|
|
Galactic longitude (°) |
84.9635Ref |
Proper motion in α (mas/yr) |
-3.18±0.04Ref |
|
|
Galactic latitude (°) |
2.2035Ref |
Proper motion in δ (mas/yr) |
-5.02±0.04Ref |
|
|
Observations
X-Ray |
- |
IR type |
S?Ref |
Radio |
- |
X-Ray type |
- |
J (mag) |
9.55Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
8.09Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
7.50Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
7.13Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
7.27Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
7.05Ref |
IPmax (eV) |
- |
B (mag) |
- |
WISE W4 (mag) |
7.04Ref |
[O III] lines |
- |
V (mag) |
15.24Ref |
IRAS 12μm (Jy) |
- |
He II lines |
- |
R (mag) |
- |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
- |
I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
- |
BP (mag) |
17.90Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
14.39Ref |
AKARI S09 (Jy) |
0.11Ref |
|
|
RP (mag) |
12.87Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
- |
γ velocity (km/h) |
-99.60±0.96Ref |
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 |
S?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 |
- |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Classified as a compact PN resembling a late-type star (class S) by Allen (1974), who also suggested that most objects in this class are symbiotics or VV Cep-type stars. Subsequent observations in Acker & Stenholm (1990) identified the object as an M-type star.
References
- Acker, A., Stenholm, B., 1990, A&AS, 86, 219, 1990A&AS...86..219A
- Allen, D. A., 1974, MNRAS, 168, 1, 1974MNRAS.168....1A
Last updated: April 30, 2022