CONFIRMED M33
Equatorial coordinates
α = 23.350196 | 01 33 24.047000
δ = 30.426272 | +30 25 34.580000 |
|
Constellation |
Triangulum |
Symbiotic IR Type |
|
Spectral Type |
yellow/red hypergiant + O-B |
Magnitude range (V) |
|
Outbursts |
No |
|
|
Identifiers
Position
Right ascension (°) |
23.350196 |
Parallax (mas) |
– |
Reddening E(B-V) (mag) |
0.039 ± 0.001 |
Declination (°) |
30.426272 |
Distance (kpc) |
847.00 ± 60.00 |
|
|
Galactic longitude (°) |
133.551679 |
Proper motion in α (mas/yr) |
– |
|
|
Galactic latitude (°) |
-31.578679 |
Proper motion in δ (mas/yr) |
– |
|
|
Observations
U (mag) |
>24.1 |
X-Ray |
|
Flickering |
|
B (mag) |
>24.2 |
X-Ray type |
|
Outbursts |
No |
V (mag) |
23.15 |
IUE |
No |
Type |
|
R (mag) |
21.61 |
IRAS flux at 12 μm (Jy) |
|
IPmax (eV) |
35.1 |
I (mag) |
19.99 |
IRAS flux at 25 μm (Jy) |
|
OVI lines |
No |
G (mag) |
|
IRAS flux at 60 μm (Jy) |
|
|
|
J (mag) |
17.07 |
IRAS flux at 100 μm (Jy) |
|
|
|
H (mag) |
15.04 |
WISE W1 (mag) |
11.95 |
|
|
K (mag) |
13.60 |
WISE W2 (mag) |
10.80 |
|
|
L (mag) |
|
WISE W3 (mag) |
7.91 |
|
|
|
|
WISE W4 (mag) |
5.30 |
|
|
|
|
Radio |
|
|
|
|
|
Radio flux (mJy) |
|
|
|
Orbit
Orbital period (days) |
>10957500 |
γ velocity (km/h) |
-113 |
Size of giant’s orbit (AU) |
|
Eccentricity |
|
RV of giant (km/h) |
|
Separation (AU) |
|
Inclination (°) |
|
Inferior conj. of giant (JD) |
|
Mass function |
|
Ephemeris type |
|
|
|
Mass ratio |
|
Ephemeris T0 (JD) |
|
|
|
|
|
Cool component
Spectral type |
yellow/red hypergiant |
Mass (M⊙) |
>30 |
Pulsation |
|
Eff. temperature (K) |
|
Radius (R⊙) |
|
Type |
|
IR type |
|
Luminosity (L⊙) |
|
Pulsation period (days) |
|
Metallicity [Fe/H] |
|
|
|
Ephemeris type |
|
|
|
|
|
Ephemeris T0 (JD) |
|
Hot component
Type/Spectra |
O-B |
Mass (M⊙) |
20-30 |
Spin period (min) |
|
Eff. temperature (K) |
|
Radius (R⊙) |
|
Accretion disk |
|
Lower limit (K) |
35000 |
Luminosity (L⊙) |
80000-160000 |
|
|
Upper limit (K) |
45000 |
|
|
|
|
Links
SIMBAD CDS Portal
Notes
The most luminous infrared star in M33. The star is clearly composite, with a hot, luminous O-B star component and a cool, dust-enshrouded companion. Object X is a very young and massive binary star (Mikołajewska et al., 2015).
References
- Khan, R., Stanek, K. Z., Kochanek, C. S., et al., 2011, ApJ, 732, 43, 2011ApJ…732…43K
- Mikołajewska, J., Caldwell, N., Shara, M. M., et al., 2015, ApJ, 799, L16, 2015ApJ…799L..16M
Last updated: Jan 14, 2019 @ 9:21 am