PM 2-14
SUSPECTED
MILKY WAY
Constellation
Centaurus |
Equatorial coordinates
α = 13 46 20.581
δ = -62 47 59.780 |
Galactic coordinates
l = 309.1589°
b = -0.5939° |
| Suspected |
2016Ref |
| Confirmed |
- |
| Symbiotic IR type |
D?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 (°) |
206.5858Ref |
Parallax (mas) |
- |
Reddening E(B-V) (mag) |
12.16±2.1Ref, Note |
| Declination (°) |
-62.7999Ref |
Distance (kpc) |
-, Note |
|
|
| Galactic longitude (°) |
309.1589Ref |
Proper motion in α (mas/yr) |
- |
|
|
| Galactic latitude (°) |
-0.5939Ref |
Proper motion in δ (mas/yr) |
- |
|
|
Observations
| X-Ray |
NoRef |
IR type |
D?Ref |
Radio |
NoRef |
| X-Ray type |
- |
J (mag) |
12.74Ref |
Flickering |
- |
| GALEX FUV (mag) |
- |
H (mag) |
11.96Ref |
Outbursts |
- |
| GALEX NUV (mag) |
- |
K (mag) |
10.67Ref |
Outburst type |
- |
| IUE |
NoRef |
WISE W1 (mag) |
6.72Ref |
Jets |
- |
| FUSE |
NoRef |
WISE W2 (mag) |
5.00Ref |
Resolved nebula |
YesRef |
| U (mag) |
- |
WISE W3 (mag) |
0.25Ref |
IPmax (eV) |
13.6Ref |
| B (mag) |
- |
WISE W4 (mag) |
-3.50Ref |
[O III] lines |
NoRef |
| V (mag) |
- |
IRAS 12μm (Jy) |
21.90Ref |
He II lines |
NoRef |
| R (mag) |
- |
IRAS 25μm (Jy) |
337.00Ref |
[Fe VII] lines |
NoRef |
| I (mag) |
- |
IRAS 60μm (Jy) |
395.00Ref |
O VI lines |
NoRef |
| BP (mag) |
- |
IRAS 100μm (Jy) |
186.00Ref |
|
|
| G (mag) |
- |
AKARI S09 (Jy) |
8.53Ref |
|
|
| RP (mag) |
- |
AKARI S18 (Jy) |
179.50Ref |
|
|
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 |
CRef |
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 |
- |
Radius (R⊙) |
- |
Accretion disk |
- |
| Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
| Lower limit (K) |
- |
|
|
|
|
| Upper limit (K) |
- |
|
|
|
|
Notes
Classified as a symbiotic star candidate in the HASH Database of PNe (Parker et al., 2016), this object exhibits an hourglass-shaped nebula. The spectrum reveals only Hα. It has been also proposed as a possible carbon star (Siódmiak et al., 2008).
References
- Parker, Q. A., Bojičić, I. S., Frew, D. J., 2016, JPhCS, 728, 3, 032008, 2016JPhCS.728c2008P
- Siódmiak, N., Meixner, M., Ueta, T. et al., 2008, ApJ, 677, 1, 382, 2008ApJ...677..382S
Last updated: March 25, 2022