New Online Database of Symbiotic Variables: Mz 3

Constellation
Norma

Equatorial coordinates
α = 16 17 13.385
δ = -51 59 10.775

Galactic coordinates
l = 331.7274°
b = -1.0114°

Suspected	2001^Ref
Confirmed	-
Symbiotic IR type	D?^Ref
Hot component type	-
Outbursts	-

Identifiers

Mz 3	IRAS 16133-5151	GSC2.4.2 S8T9403434	AAVSO -
SIMBAD PN Mz 3	Pan-STARRS -	SAO -	VSX -
GAIA DR3 5934701559547878144	SkyMapper 161713.38-515910.6	WRAY 16-213	GCVS -
2MASS J16171340-5159106	HIP -	Hen 2-154	BD -
WISE J161713.40-515910.7	TYC -	ESO 225-9	HD -

Symbiotic Catalogs

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

Position

Right ascension (°)	244.3058^Ref	Parallax (mas)	0.366±0.086^Ref	Reddening E(B-V) (mag)	1.76±0.07^Ref ^{, Note}
Declination (°)	-51.9863^Ref	Distance (kpc)	2.65^Ref ^{, Note}, 2.31^Ref ^{, Note}
Galactic longitude (°)	331.7274^Ref	Proper motion in α (mas/yr)	-3.55±0.10^Ref
Galactic latitude (°)	-1.0114^Ref	Proper motion in δ (mas/yr)	-3.91±0.08^Ref

Observations

X-Ray	Yes^Ref	IR type	D?^Ref	Radio	Yes^Ref
X-Ray type	-	J (mag)	9.35^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	7.36^Ref	Outbursts	-
GALEX NUV (mag)	-	K (mag)	5.61^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	3.25^Ref	Jets	Yes^Ref
FUSE	No^Ref	WISE W2 (mag)	0.46^Ref	Resolved nebula	Yes^Ref
U (mag)	-	WISE W3 (mag)	-0.97^Ref	IPmax (eV)	35.1^Ref
B (mag)	10.80^Ref	WISE W4 (mag)	-4.46^Ref	[O III] lines	Yes^Ref
V (mag)	14.00^Ref	IRAS 12μm (Jy)	88.80^Ref	He II lines	No^Ref
R (mag)	-	IRAS 25μm (Jy)	343.00^Ref	[Fe VII] lines	No^Ref
I (mag)	-	IRAS 60μm (Jy)	277.00^Ref	O VI lines	No^Ref
BP (mag)	13.76^Ref	IRAS 100μm (Jy)	113.00^Ref
G (mag)	13.19^Ref	AKARI S09 (Jy)	55.32^Ref
RP (mag)	12.00^Ref	AKARI S18 (Jy)	267.90^Ref

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	-	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)	-

Links

SIMBAD CDS Portal

Notes

The central star of the planetary nebula Mz 3 is not resolved, and a potential symbiotic nature of its core was proposed by Schmeja & Kimeswenger (2001). Additionally, fast outflows have been observed in the object (Redman et al., 2000).

References

Clyne, N., Akras, S., Steffen, W. et al., 2015, A&A, 582, A60, 2015A&A...582A..60C
Redman, M. P., O´Connor, J. A., Holloway, A. J. et al., 2000, MNRAS, 312, 2, L23, 2000MNRAS.312L..23R
Schmeja, S., Kimeswenger, S., 2001, A&A, 377, L18, 2001A&A...377L..18S
Smith, N., 2003, MNRAS, 342, 2, 383, 2003MNRAS.342..383S
Zhang, Y., Liu, X.-W., 2002, MNRAS, 337, 2, 499, 2002MNRAS.337..499Z

Mz 3