CXOM31 J003825.7+401739

SUSPECTED M31   Equatorial coordinates α =  9.607053 ± 0.186900 | 00 38 25.692726  δ =  40.294083 ± 0.188000 | +40 17 38.698295   Constellation Andromeda Symbiotic IR Type   Spectral Type   Magnitude range (V)   Outbursts No

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Identifiers

CXOM31 J003825.7+401739	GSC –	TYC –	WRAY –
SIMBAD [KGP2002] s2-10	HIP –	SAO –	Hen –
BD –	IRAS –	GAIA DR2 380745174299369472	ESO –
HD –	2MASS J00382569+4017388	WISE –	AAVSO –

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Position

Right ascension (°)	9.607053 ± 0.186900refGaia Collaboration, Brown, A. G. A., Vallenari, A., et al., 2018, A&A, 616, A1, 2018A&A…616A…1G	Parallax (mas)	–	Reddening E(B-V) (mag)	0.058 ± 0.005refSchlafly, E. F., Finkbeiner, D. P., 2011, ApJ, 737, 103, 2011ApJ…737..103S
Declination (°)	40.294083 ± 0.188000refGaia Collaboration, Brown, A. G. A., Vallenari, A., et al., 2018, A&A, 616, A1, 2018A&A…616A…1G	Distance (kpc)	785.00 ± 25.00refMcConnachie, A. W., Irwin, M. J., Ferguson, A. M. N., et al., 2005, MNRAS, 356, 979, 2005MNRAS.356..979M
Galactic longitude (°)	120.247055 ± 0.188000refGaia Collaboration, Brown, A. G. A., Vallenari, A., et al., 2018, A&A, 616, A1, 2018A&A…616A…1G	Proper motion in α (mas/yr)	–
Galactic latitude (°)	-22.509836 ± 0.186900refGaia Collaboration, Brown, A. G. A., Vallenari, A., et al., 2018, A&A, 616, A1, 2018A&A…616A…1G	Proper motion in δ (mas/yr)	–

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Observations

U (mag)		X-Ray	YesrefDi Stefano, R., Kong, A. K. H., Greiner, J., et al., 2004, ApJ, 610, 247, 2004ApJ…610..247D	Flickering
B (mag)	21.10refDi Stefano, R., Kong, A. K. H., Greiner, J., et al., 2004, ApJ, 610, 247, 2004ApJ…610..247D	X-Ray type		Outbursts	No
V (mag)	19.40refDi Stefano, R., Kong, A. K. H., Greiner, J., et al., 2004, ApJ, 610, 247, 2004ApJ…610..247D	IUE	No	Type
R (mag)		IRAS flux at 12 μm (Jy)		IPmax (eV)
I (mag)		IRAS flux at 25 μm (Jy)		OVI lines
G (mag)	18.13refGaia Collaboration, Brown, A. G. A., Vallenari, A., et al., 2018, A&A, 616, A1, 2018A&A…616A…1G	IRAS flux at 60 μm (Jy)
J (mag)	15.09refCutri, R. M., Skrutskie, M. F., van Dyk, S., et al., 2003, VizieR On-line Data Catalog: II/246, 2003yCat.2246….0C	IRAS flux at 100 μm (Jy)
H (mag)	14.61refCutri, R. M., Skrutskie, M. F., van Dyk, S., et al., 2003, VizieR On-line Data Catalog: II/246, 2003yCat.2246….0C	WISE W1 (mag)	14.14refCutri, R. M., et al., 2014, I II/328, 2014yCat.2328….0C
K (mag)	14.26refCutri, R. M., Skrutskie, M. F., van Dyk, S., et al., 2003, VizieR On-line Data Catalog: II/246, 2003yCat.2246….0C	WISE W2 (mag)	14.00refCutri, R. M., et al., 2014, I II/328, 2014yCat.2328….0C
L (mag)		WISE W3 (mag)	12.39refCutri, R. M., et al., 2014, I II/328, 2014yCat.2328….0C
		WISE W4 (mag)	8.87refCutri, R. M., et al., 2014, I II/328, 2014yCat.2328….0C
		Radio
		Radio flux (mJy)

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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
Ephemeris type				Mass ratio
Ephemeris T0 (JD)

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Cool component

Spectral type		Mass (M⊙)		Pulsation
Eff. temperature (K)		Radius (R⊙)		Type
IR type		Luminosity (L⊙)		Pulsation period (days)
Metallicity [Fe/H]				Ephemeris type
				Ephemeris T0 (JD)

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Hot component

Type/Spectra		Mass (M⊙)		Spin period (min)
Eff. temperature (K)		Radius (R⊙)		Accretion disk
Lower limit (K)		Luminosity (L⊙)
Upper limit (K)

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Links

SIMBAD     CDS Portal

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Notes

Identified as an X-ray source in M31. Di Stefano et al. (2004) identified the object as a possible symbiotic system, they also identified an optical counterpart.

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References

• Di Stefano, R., Kong, A. K. H., Greiner, J., et al., 2004, ApJ, 610, 247, 2004ApJ…610..247D

Last updated: May 12, 2019 @ 7:56 pm