New Online Database of Symbiotic Variables: M33SyS J013303.27+303528.3

CONFIRMED M33

Constellation
Triangulum

Equatorial coordinates
α = 01 33 03.234
δ = +30 35 28.074

Galactic coordinates
l = 133.4290°
b = -31.4309°

Suspected	2017^Ref
Confirmed	2017^Ref
Symbiotic IR type	-
Hot component type	shell-burning^Ref
Outbursts	-

Identifiers

M33SyS J013303.27+303528.3	IRAS 01301+3019	GSC2.4.2 NBXZ001819	AAVSO -
SIMBAD M33SyS J013303.27+303528.3	Pan-STARRS 144700232634349894	SAO -	VSX -
GAIA DR3 303287775579028736	SkyMapper -	WRAY -	GCVS -
2MASS -	HIP -	Hen -	BD -
WISE J013303.21+303525.9	TYC -	ESO -	HD -

Symbiotic Catalogs

Bidelman (1954)	-	Allen (1984)	-	Belzcyński et al. (2001)	-
Gaposchkin (1957)	-	Kenyon (1986)	-	Akras et al. (2019)	M33 SySt-3 (Conf.)
Boyarchuk (1969)	-	Vaidis (1988, 1991)	-

Position

Right ascension (°)	23.2635^Ref	Parallax (mas)	-	Reddening E(B-V) (mag)	0.04±0.0^Ref ^{, Note}
Declination (°)	30.5911^Ref	Distance (kpc)	847±60^Ref -^{, Note}
Galactic longitude (°)	133.4290^Ref	Proper motion in α (mas/yr)	-
Galactic latitude (°)	-31.4309^Ref	Proper motion in δ (mas/yr)	-

Observations

X-Ray	No^Ref	IR type	-	Radio	-
X-Ray type	-	J (mag)	-	Flickering	-
GALEX FUV (mag)	-	H (mag)	-	Outbursts	-
GALEX NUV (mag)	-	K (mag)	-	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	15.31^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	15.84^Ref	Resolved nebula	-
U (mag)	23.52^Ref	WISE W3 (mag)	12.65^Ref	IPmax (eV)	114^Ref
B (mag)	23.79^Ref	WISE W4 (mag)	9.23^Ref	[O III] lines	Yes^Ref
V (mag)	22.12^Ref	IRAS 12μm (Jy)	0.38^Ref	He II lines	Yes^Ref
R (mag)	20.74^Ref	IRAS 25μm (Jy)	0.29^Ref	[Fe VII] lines	Yes^Ref
I (mag)	19.58^Ref	IRAS 60μm (Jy)	0.97^Ref	O VI lines	Yes^Ref
BP (mag)	21.10^Ref	IRAS 100μm (Jy)	4.89^Ref
G (mag)	20.84^Ref	AKARI S09 (Jy)	-
RP (mag)	19.73^Ref	AKARI S18 (Jy)	-

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	CN^Ref	Mass (M_⊙)	-	Pulsation	Yes^Ref
Eff. temperature (K)	-	Radius (R_⊙)	-	Type	low-amplitude SR^Ref
IR type	-	Luminosity (L_⊙)	-	Pulsation period (days)	100^Ref
Metallicity [Fe/H]	-			Pulsation ephemeris	-

Hot component

Type/Spectral type	-	Mass (M_⊙)	-	Spin period (min)	-
Shell-burning/Accreting-only	shell-burning^Ref	Radius (R_⊙)	-	Accretion disk	-
Eff. temperature (K)	-	Luminosity (L_⊙)	-
Lower limit (K)	114000^Ref
Upper limit (K)	176000^Ref

Links

SIMBAD CDS Portal

Notes

The light curves of M33SyS J013303.27+303528.3 appear to be dominated by red giant pulsations, with a period of approximately 100 days (Mikołajewska et al., 2017).

References

Mikołajewska, J., Shara, M. M., Caldwell, N. et al., 2017, MNRAS, 465, 2, 1699, 2017MNRAS.465.1699M

M33SyS J013303.27+303528.3