LMC N67

CONFIRMED LMC

Constellation
Dorado

Equatorial coordinates
α = 05 36 07.580
δ = -64 43 21.333

Galactic coordinates
l = 274.3535°
b = -32.3418°

Suspected	1989^Ref
Confirmed	1989^Ref
Symbiotic IR type	S^Ref
Hot component type	shell-burning^Ref
Outbursts	-

Identifiers

LMC N67	IRAS -	GSC2.4.2 S13G006427	AAVSO 000-BLT-634
SIMBAD LHA 120-N 67	Pan-STARRS -	SAO -	VSX 410502
GAIA DR3 4756944805986367744	SkyMapper 053607.60-644321.8	WRAY -	GCVS -
2MASS J05360754-6443212	HIP -	Hen -	BD -
WISE J053607.57-644321.4	TYC -	ESO -	HD -

Symbiotic Catalogs

Bidelman (1954)	-	Allen (1984)	-	Belzcyński et al. (2001)	LMC N67 (Conf.)
Gaposchkin (1957)	-	Kenyon (1986)	-	Akras et al. (2019)	LMC N67 (Conf.)
Boyarchuk (1969)	-	Vaidis (1988, 1991)	LMC C495 (Conf.)

Position

Right ascension (°)	84.0316^Ref	Parallax (mas)	-0.029±0.026^Ref	Reddening E(B-V) (mag)	0.05±0.0^Ref ^{, Note}
Declination (°)	-64.7226^Ref	Distance (kpc)	49.97±0.19^Ref 17.07^Ref ^{, Note}, 10.52^Ref ^{, Note}
Galactic longitude (°)	274.3535^Ref	Proper motion in α (mas/yr)	1.51±0.04^Ref
Galactic latitude (°)	-32.3418^Ref	Proper motion in δ (mas/yr)	0.34±0.03^Ref

Observations

X-Ray	No^Ref	IR type	S^Ref	Radio	-
X-Ray type	-	J (mag)	12.67^Ref	Flickering	-
GALEX FUV (mag)	18.22^Ref	H (mag)	11.85^Ref	Outbursts	-
GALEX NUV (mag)	19.10^Ref	K (mag)	11.46^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	11.08^Ref	Jets	-
FUSE	Yes^Ref	WISE W2 (mag)	11.12^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	10.61^Ref	IPmax (eV)	114^Ref
B (mag)	16.18^Ref	WISE W4 (mag)	9.58^Ref	[O III] lines	No^Ref
V (mag)	15.35^Ref	IRAS 12μm (Jy)	-	He II lines	Yes^Ref
R (mag)	14.70^Ref	IRAS 25μm (Jy)	-	[Fe VII] lines	No^Ref
I (mag)	12.70^Ref	IRAS 60μm (Jy)	-	O VI lines	Yes^Ref
BP (mag)	16.04^Ref	IRAS 100μm (Jy)	-
G (mag)	15.21^Ref	AKARI S09 (Jy)	-
RP (mag)	14.30^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	Yes?^Ref			Mass ratio	-
Orbital ephemeris	-

Cool component

Spectral type	C3.2^Ref	Mass (M_⊙)	-	Pulsation	Yes^Ref
Eff. temperature (K)	3350^Ref	Radius (R_⊙)	170^Ref	Type	OGLE Small Amplitude Red Giant^Ref
IR type	S^Ref	Luminosity (L_⊙)	3300^Ref	Pulsation period (days)	45±5^Ref
Metallicity [Fe/H]	-			Pulsation ephemeris	Min(I) = 2455513±1 + 45±5 x E^Ref

Hot component

Type/Spectral type	-	Mass (M_⊙)	-	Spin period (min)	-
Shell-burning/Accreting-only	shell-burning^Ref	Radius (R_⊙)	0.082^Ref	Accretion disk	-
Eff. temperature (K)	130000±30000^Ref, 100000-160000^Ref	Luminosity (L_⊙)	2000±1000^Ref, 800-3000^Ref
Lower limit (K)	-
Upper limit (K)	-

Links

SIMBAD CDS Portal

Notes

LMC N67 is identified as a carbon symbiotic star. In Angeloni et al. (2014), it was noted that the observed light curve likely exhibits eclipses.

References

Akras, S., Guzman-Ramirez, L., Leal-Ferreira, M. L. et al., 2019, ApJS, 240, 2, 21, 2019ApJS..240...21A
Angeloni, R., Ferreira Lopes, C. E., Masetti, N. et al., 2014, MNRAS, 438, 1, 35, 2014MNRAS.438...35A
Cowley, A. P., Hartwick, F. D. A., 1989, PASP, 101, 917, 1989PASP..101..917C
Morgan, D. H., 1992, MNRAS, 258, 639, 1992MNRAS.258..639M
Mürset, U., Schild, H., Vogel, M., 1996, A&A, 307, 516, 1996A&A...307..516M
Vogel, M., Morgan, D. H., 1994, A&A, 288, 842, 1994A&A...288..842V

Last updated: May 2, 2019