Y CrA
CONFIRMED
MILKY WAY
Constellation
Corona Australis |
Equatorial coordinates
α = 18 14 22.947
δ = -42 50 32.335 |
Galactic coordinates
l = 350.6096°
b = -11.8301° |
Suspected |
1954Ref |
Confirmed |
1978Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
Y CrA (Conf.) |
Allen (1984) |
Y CrA (Conf.) |
Belzcyński et al. (2001) |
Y CrA (Conf.) |
Gaposchkin (1957) |
- |
Kenyon (1986) |
Y CrA (Conf.) |
Akras et al. (2019) |
Y CrA (Conf.) |
Boyarchuk (1969) |
Y CrA (Susp.) |
Vaidis (1988, 1991) |
Y CrA (Conf.) |
Position
Right ascension (°) |
273.5956Ref |
Parallax (mas) |
0.278±0.034Ref |
Reddening E(B-V) (mag) |
0.12±0.0Ref, Note |
Declination (°) |
-42.8423Ref |
Distance (kpc) |
5Ref 3.42Ref, Note, 3.51Ref, Note |
|
|
Galactic longitude (°) |
350.6096Ref |
Proper motion in α (mas/yr) |
-2.42±0.04Ref |
|
|
Galactic latitude (°) |
-11.8301Ref |
Proper motion in δ (mas/yr) |
-0.98±0.03Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
SRef |
Radio |
YesRef |
X-Ray type |
- |
J (mag) |
7.77Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
6.84Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
6.48Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
6.31Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
6.25Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
5.94Ref |
IPmax (eV) |
114Ref |
B (mag) |
- |
WISE W4 (mag) |
5.55Ref |
[O III] lines |
YesRef |
V (mag) |
13.30Ref |
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) |
13.13Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
11.56Ref |
AKARI S09 (Jy) |
0.22Ref |
|
|
RP (mag) |
10.23Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
1619±35.8Ref |
γ velocity (km/h) |
-49.04±0.31Ref, -48.68±2.20Ref |
Size of giant’s orbit (AU) |
0.8Ref |
Eccentricity |
0.173±0.088Ref |
RV of giant (km/h) |
5.55±0.43Ref |
Separation (AU) |
- |
Inclination (°) |
- |
Inferior conj. of giant (JD) |
- |
Mass function |
0.0275Ref |
Eclipses |
- |
|
|
Mass ratio |
- |
Orbital ephemeris |
- |
|
|
|
|
Cool component
Spectral type |
M5 IIIRef, M6 IIIRef, M6 IIIRef |
Mass (M⊙) |
- |
Pulsation |
YesRef |
Eff. temperature (K) |
3235Ref, 3300Ref |
Radius (R⊙) |
- |
Type |
SRRef |
IR type |
SRef |
Luminosity (L⊙) |
- |
Pulsation period (days) |
84±1Ref |
Metallicity [Fe/H] |
-0.4±0.06Ref |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
- |
Mass (M⊙) |
- |
Spin period (min) |
- |
Shell-burning/Accreting-only |
shell-burningRef |
Radius (R⊙) |
0.011Ref |
Accretion disk |
- |
Eff. temperature (K) |
130000-140000Ref, 190000Ref |
Luminosity (L⊙) |
260Ref, 140Ref |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
References
- Allen, D. A., 1978, MNRAS, 184, 601, 1978MNRAS.184..601A
- Allen, D. A., 1980, MNRAS, 192, 521, 1980MNRAS.192..521A
- Bidelman, W. P., 1954, ApJS, 1, 175, 1954ApJS....1..175B
- Cannon, A. J., Pickering, E. C., 1916, AnHar, 76, 3, 19, 1916AnHar..76...19C
- Fekel, F. C., Hinkle, K. H., Joyce, R. R. et al., 2010, AJ, 139, 4, 1315, 2010AJ....139.1315F
- Fleming, W. P. S., Pickering, E. C., 1912, AnHar, 56, 6, 165, 1912AnHar..56..165F
- Gałan, C., Mikołajewska, J., Hinkle, K. H. et al., 2016, MNRAS, 455, 2, 1282, 2016MNRAS.455.1282G
- Gromadzki, M., Mikołajewska, J., Soszyński, I., 2013, AcA, 63, 4, 405, 2013AcA....63..405G
- Gutiérrez-Moreno, A., Moreno, H., Costa, E., 1999, PASP, 111, 759, 571, 1999PASP..111..571G
- Henize, K. G., 1967, ApJS, 14, 125, 1967ApJS...14..125H
- 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
- Mürset, U., Schmid, H. M., 1999, A&AS, 137, 473, 1999A&AS..137..473M
- Payne, C. H., 1930, BHarO, 878, 1, 1930BHarO.878....1P
- Pickering, E. C., Colson, H. R., Fleming, W. P. et al., 1901, ApJ, 13, 226, 1901ApJ....13..226P
- Sanduleak, N., Stephenson, C. B., 1973, ApJ, 185, 899, 1973ApJ...185..899S
Last updated: April 18, 2022