V417 CMa

CONFIRMED MILKY WAY
 
Constellation
Canis Major
Equatorial coordinates
α = 07 01 09.154
δ = -29 06 24.983
Galactic coordinates
l = 240.1934°
b = -10.8862°

Suspected 2000Ref
Confirmed 2002Ref
Symbiotic IR type SRef
Hot component type accreting-onlyRef
Outbursts -

Identifiers

V417 CMa IRAS 06591-2902 GSC2.4.2 S3G0000673 AAVSO 000-BGH-634
SIMBAD CD-28 3719 Pan-STARRS 73071052881351922 SAO - VSX 81842
GAIA DR3 5608089951177429120 SkyMapper 070109.15-290625.0 WRAY 18-5 GCVS V0417 CMa
2MASS J07010915-2906250 HIP - Hen 4-18 BD -
WISE J070109.17-290625.1 TYC 6535-2424-1 ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) - Belzcyński et al. (2001) CD-28 3719 (Susp.)
Gaposchkin (1957) - Kenyon (1986) - Akras et al. (2019) Hen 4-18 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) -

Position

Right ascension (°) 105.2881Ref Parallax (mas) 0.575±0.022Ref Reddening E(B-V) (mag) 0.11±0.0Ref, Note
Declination (°) -29.1069Ref Distance (kpc) 1.65Ref, Note, 1.67Ref, Note    
Galactic longitude (°) 240.1934Ref Proper motion in α (mas/yr) -1.22±0.02Ref    
Galactic latitude (°) -10.8862Ref Proper motion in δ (mas/yr) 3.95±0.02Ref    

Observations

X-Ray YesRef IR type SRef Radio NoRef
X-Ray type δRef J (mag) 6.12Ref Flickering YesRef
GALEX FUV (mag) - H (mag) 5.27Ref Outbursts -
GALEX NUV (mag) - K (mag) 4.92Ref Outburst type -
IUE NoRef WISE W1 (mag) 4.91Ref Jets -
FUSE NoRef WISE W2 (mag) 4.85Ref Resolved nebula -
U (mag) - WISE W3 (mag) 4.81Ref IPmax (eV) 13.6Ref
B (mag) 12.15Ref WISE W4 (mag) 4.64Ref [O III] lines -
V (mag) 10.61Ref IRAS 12μm (Jy) 0.53Ref He II lines -
R (mag) - IRAS 25μm (Jy) 0.25Ref [Fe VII] lines -
I (mag) - IRAS 60μm (Jy) 0.40Ref O VI lines -
BP (mag) 10.85Ref IRAS 100μm (Jy) 1.09Ref
G (mag) 9.21Ref AKARI S09 (Jy) 0.67Ref
RP (mag) 7.99Ref AKARI S18 (Jy) -

Orbit

Orbital period (days) - γ velocity (km/h) 67.43±1.61Ref 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 S6.8Ref Mass (M) - Pulsation YesRef
Eff. temperature (K) - Radius (R) - Type SRRef
IR type SRef Luminosity (L) - Pulsation period (days) 198±3Ref
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

Type/Spectral type - Mass (M) - Spin period (min) -
Shell-burning/Accreting-only accreting-onlyRef Radius (R) - Accretion disk -
Eff. temperature (K) - Luminosity (L) -    
Lower limit (K) -        
Upper limit (K) -        

Links

SIMBAD   CDS Portal   ARAS Database


Notes

S-type star (Stephenson, 1984). Initially classified as a possible symbiotic star by Belczyński et al. (2000), based on private communication with A. Jorissen. The system exhibits a broad Hα profile and blue colors (van Eck & Jorissen, 2002).


References


Last updated: January 12, 2024