WDS 05074+1839 A 3010 AB : NOTES
 
 
discov_num notes refcode
A 3010 104 Tau.
Two orbit solutions (Eggen 1956). Observations of this close pair Egg1956
are so scattered that both orbits are highly conjectural.
A measure on 1977.9196 was incorrectly attributed to ADS 3701 in
McAlister & Hendry (1982); it actually belongs to ADS 4020. McA1982b
Visual and speckle observations at 0".1 sep ruled out as spurious by
constant RV (Duquennoy & Mayor 1991). Duq1991
Precise velocities are stable to better than 100 m/s over 388 days, Nid2002
so there are no "hot jupiters" and a 2-year period is excluded with Tok2010b
high confidence.
104 Tau is a G4V dwarf at 16 pc resolved into equal components at 0.1"
by R. Aitken in 1912. The WDS contains 16 resolutions of this pair. A__1927a
Apart from Aitken himself, it has been resolved on multiple occasions
by R.H. Wilson in 1934-1971, by W. Finsen (1953-1955) and by others, WRH1941a
although in other instances those observers found it to be single. Fin1953d
The measures suggest a near-circular orbit seen face-on with a semi-
major axis on the order of 0.1" or 1.5 au. Assuming a mass sum of 2
Msun, the orbital period should be around 1.3 yr; in fact, two orbits
with periods 1.19 yr and 2.38 yr were published by Eggen (1956). This Egg1956
binary should be an easy target for speckle interferometry at 4-m
telescopes. It was observed 10 times from 1976.9 to 1980.7 with
speckle and, surprisingly, found unresolved on all occasions,
excluding any short-period orbits. Later, however, two measures were
made by the author at a 1-m telescope with a phase-grating
interferometer. The first resolution in 1984.8 at 0.04" was tentative Tok1985
(below the diffraction limit), but the second in 1985.7 was secure, Tok1988
being an average of two observations. It was followed by the speckle
resolution at 4-m telescope in 1988.17, after which the pair Mca1993
disappeared again. It was found unresolved in 2012. Tok2012b
The star is well studied. Two statistical surveys of binaries within
25 pc consider it to be single (Duquennoy & Mayor 1991; Raghavan et Duq1991
al. 2010). Heintz & Borgman (1984) state that measures cannot be Rag2010
fitted by any orbit and conclude: "Although this alleged visual binary Hei1984i
(ADS 3701) has three published orbits, it is probably spurious".
Several independent RV studies have shown that this star is not a
spectroscopic binary. Precise RVs measured by Nidever et al. (2002) Nid2002
are stable to better than 100 m s-1 over 388 days, excluding orbital
periods from one to two years with high confidence. Data with lower
precision show a constant RV of +21 km/s over many years (Duquennoy &
Mayor 1991; Abt & Willmarth 2006; Raghavan et al. 2010). The star is AbH2006
located about 1m above the main sequence, supporting the thesis of an
equal-component binary. If the orbit is seen face-on, the RV variation
would be small, especially if the components are of equal brightness
(blended lines move in opposite directions, the centroid stays
constant). However, the lines in this star remain narrow and the
speckle non-resolution during 3.8 yr firmly excludes a face-on orbit.
Remember that 104 Tau is bright (no identification errors possible)
and that the components are supposedly equally bright, hence easy to
resolve by speckle. If this star is single (as everything seems to
suggest), we cannot dismiss its multiple resolutions with micrometer,
eyepiece interferometer, and speckle as spurious; occasional image
doubling (or at least elongation) must be real. Tok2012b
Ghost binary. Tok2012b
Malkov et al. (2012) derive dynamical, photometric, and spectroscopic
masses of 0.65 +/- 0.09, 2.12, and 1.02 Msun, respectively. Mlk2012
In the WDS summary line this carries an "X" code (non double), but
still retains all the historical measures.
 
 
REFERENCES
 
 
refcode metd author reference
A__1927a Ma - Aitken, R.G. 1927LicOB..12..170A
A__1927a Lick Obs. Bull. 12, 170, 1927
AbH2006 orb - Abt, H.A., & Willmarth, D. 2006ApJS..162..207A
AbH2006 ApJS 162, 207, 2006
Duq1991 - Duquennoy, A. & Mayor, M. 1991A&A...248..485D
Duq1991 A&A 248, 485, 1991
Egg1956 orb - Eggen, O.J. 1956AJ.....61..405E
Egg1956 AJ 61, 405, 1956
Fin1953d J - Finsen, W.S. 1953CiUO..113..170F
Fin1953d Union Obs. Johannesburg Circ. 113, 170, 1953
Hei1984i Po - Heintz, W.D. & Borgman, E.R. 1984AJ.....89.1068H
Hei1984i AJ 89, 1068, 1984
McA1982b Sc j McAlister, H.A. & Hendry, E.M. 1982ApJS...48..273M
McA1982b ApJS 48, 273, 1982
McA1993 Sc j McAlister, H.A., Mason, B.D., Hartkopf, W.I., & Shara, M.M. 1993AJ....106.1639M
McA1993 +orb AJ 106, 1639, 1993
Mlk2012 not - Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. 2012A&A...546A..69M
Mlk2012 A&A 546, A69, 2012
Nid2002 rv - Nidever, D.L., Marcy, G.W., Butler, R.P., Fischer, D.A., & Vogt, S.S. 2002ApJS..141..503N
Nid2002 ApJS 141, 503, 2002
Rag2010 K - Raghavan, D., McAlister, H.A., Henry, T.J., Latham, D.W., Marcy, G.W., 2010ApJS..190....1R
Rag2010 +S Mason, B.D., Gies, D.R., White, R.J. & ten Brummelaar, T.A.
Rag2010 +P ApJS 190, 1, 2010
Tok1985 Ig u Tokovinin, A.A. 1985A&AS...61..483T
Tok1985 A&AS 61, 483, 1985
Tok1988 Ig u Tokovinin, A.A. & Ismailov, R.M. 1988A&AS...72..563T
Tok1988 A&AS 72, 563, 1988
Tok2010b S - Tokovinin, A. ...................
Tok2010b private communication
Tok2012b S j Tokovinin, A. 2012AJ....144...56T
Tok2012b +orb AJ 144, 56, 2012
WRH1941a J j Wilson, R.H. 1941PFAO....6b...1W
WRH1941a +Ma Pub. Univ. Penn. 6, Pt.4, 3, 1941
WRH1941a (see also U. Penn. Flower Obs. Reprint #34, 1936)
WRH1941a (U and T coded observations per van den Bos, J Obs 34, 85, 1951) 1951JO.....34...85V
 
 
DISCOVERER
 
 
idgroup discov author
1 A Aitken, R.G.
312 HLA Hirsch, L.A., Ciardi, D.R., Howards, A.W., Marcy, G.W., Ruane, G., Gonzalez, E.,
312 HLA Blunt, S., Crepp, J.R., Fulton, B.J., Isaacson, H., Kosiarek, M., Mawet, D.,
312 HLA Sinukoff, E. & Weiss, L.
313 HLA Hirsch, L.A., Rosenthal, L., Fulton, B.J., Howard, A.W., Ciardi, D.R., Marcy, G.W.,
313 HLA Nielsen, E., Petigura, E.A., de Rosa, R.J., Isaacson, H., Weiss, L.M., Sinukoff, E.
 
 
WDS HISTORIC DATA
 
 
coord_2000 discov_num comp epoch obs pa sep mag_pri mag_sec spectr notes coord_arcsec_2000
05074+1839 A 3010 AB 1988 18 243 0.1 5.80 5.80 G1V NX 050727.00+183842.1

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