WDS 16003-2237 LAB 3 (Dschubba) : NOTES
 
 
discov_num notes refcode
LAB 3 del Sco = 7 Sco = Dschubba. A spectroscopic triple and occultation
quadruple.
Intensity Interferometer Limb-darkened diameter 0.46 +/- 0.04 mas. HBr1974
1973.22, 1973.45: The new component here appears to have a much longer
period than the 20-day single-line SB reported by van Hoof et al.
(1963 ApJ, 137, 824). Lab1974
1981.4767 and other observations through 1981.4929: Companion HBr1974
discovered by intensity interferometry (Hanbury Brown et al. 1974).
Delta m in the visible is about 2. Bag1984b
1993.415: observations with MAPPIT on 3.9m AAT; maximum separation of
apertures was 3.3m. Paper gives orbit. Bed1993
Miroshnichenko et al. (2001) give a combined spectroscopic/ Mko2001
interferometric orbit, adopting P and e from Hartkopf et al. (1996). Hrt1996a
Combined spectroscopic/astrometric solution. Tango et al. (2009) Tng2009
derive masses 15 +/- 7 and 8.0 +/- 2.6 Msun, based on their mass
function and brightness ratio, together with the ZAMS model grid of
Tout et al. (1996 MNRAS 281, 257). The resulting dynamical parallax of
7.03 +/- 0.15 mas agrees well with the revised Hipparcos parallax of
6.65 +/- 0.89 (van Leeuwen 2007, ASSL vol. 350).
Tycner et al. (2011) give a combined spectroscopic/astrometric NOI2011b
solution, based on spectroscopicdata of Miroshnichenko et al. (2001), Mko2001
published astrometry, 2 measures obtained with the NPOI array in 2000,
and 94 additional NPOI measures obtained over the years 2005-2010. The
timing of periastron passage has been revised to UT 2011 Jul 6 +/- 2d.
Expected minimum separation at closest approach is predicted to be
6.14 +/- 0.07 mas (14 stellar radii).
Malkov et al. (2012) derive dynamical and photometric masses of
28.41 +/- 11.43 and 20.39 Msun, respectively. Mlk2012
Che et al. (2012) derive an orbit of del Sco based on data from NPOI
and CHARA Array. Total mass 28 +/- 11 Msun, with the large error bar
resulting from uncertainty in parallax estimate. Individual masses
estimated at 13.9 (from photometry and spectroscopy) and ~6 Msun
(based on mass ratio from RV measurements during periastron). CIA2012c
The disk dissipates near apastron and then begins reforming as the XXX2020d
companion approaches periastron. The V magnitude is variable over the
orbit but it is unclear if this is due to the secondary or interaction
between the primary and the disk.
 
 
REFERENCES
 
 
refcode metd author reference
Bag1984b S j Balega, Y.Y., Bonneau, D., & Foy, R 1984A&AS...57...31B
Bag1984b A&AS 57, 31, 1984
Bed1993 Sa j Bedding, T.R. 1993AJ....106..768B
Bed1993 +orb AJ 106, 768, 1993
CIA2012c Kc j Che, X., Monnier, J.D., Tycner, C., Kraus, S., Zavala, R.T., Baron, F., Pedretti, 2012ApJ...757...29C
CIA2012c +orb E., ten Brummelaar, T., McAlister, H., Ridgway, S.T., Sturmann, J., Sturmann, L.,
CIA2012c & Turner, N.
CIA2012c ApJ 757, 29, 2012 (see also NOI2012)
HBr1974 - Hanbury Brown, R., Davis, J., & Allen, L.R. 1974MNRAS.167..121H
HBr1974 MNRAS 167, 121, 1974
Hrt1996a Sc j Hartkopf, W.I., Mason, B.D., & McAlister, H.A. 1996AJ....111..370H
Hrt1996a +orb AJ 111, 370, 1996
Lab1974 S j Labeyrie, A., Bonneau, D., Stachnik, R.V., & Gezari, D.Y. 1974ApJ...194L.147L
Lab1974 +orb ApJ 194, L147, 1974
Lab1974 (data from Hale 5m, KPNO 3.8m, 2.1m. Aperture listed as mean value of 3.6m unless
Lab1974 specifically given in paper)
Mko2001 orb - Miroshnichenko, A.S., Fabregat, J., Bjorkman, K.S., Knauth, D.C., Morrison, N.D., 2001A&A...377..485M
Mko2001 Tarasov, A.E., Reig, P., Negueruela, I., & Blay, P.
Mko2001 A&A 377, 485, 2001
Mlk2012 not - Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. 2012A&A...546A..69M
Mlk2012 A&A 546, A69, 2012
NOI2011b Kn j Tycner, C., Ames, A., Zavala, R.T., Hummel, C.A., Benson, J.A., & Hutter, D.J. 2011ApJ...729L...5T
NOI2011b +orb ApJL 729, 5. 2011
Tng2009 Ks - Tango, W.J., Davis, J., Jacob, A.P., Mendez, A., North, J.R., O'Byrne, J.W., 2009MNRAS.396..842T
Tng2009 +orb Seneta, E.B., & Tuthill, P.G.
Tng2009 MNRAS 396, 842, 2009
XXX2020d not - Suffak, M.W., Jones, C.E., Tycner, C., Henry, G.W., Carciofi, A.C., Mota, B.C. & 2019ApJ...890...36S
XXX2020d Rubio, A.C.
XXX2020d ApJ 890, 36, 2019
 
 
WDS HISTORIC DATA
 
 
coord_2000 discov_num comp epoch obs pa sep mag_pri mag_sec spectr notes coord_arcsec_2000
16003-2237 LAB 3 2007 44 360 0.2 2.39 4.62 Be NOD 160020.01-223717.8
16003-2237 LAB 3 2008 46 1 0.2 2.39 4.62 Be NOD 160020.01-223717.8
16003-2237 LAB 3 2010 47 13 0.1 2.39 4.62 Be NOD 160020.01-223717.8
16003-2237 LAB 3 2011 191 272 0.0 2.39 4.62 Be NO 160020.01-223717.8
16003-2237 LAB 3 2015 193 351 0.2 2.39 4.62 Be NO 160020.01-223717.8
16003-2237 LAB 3 2016 194 352 0.2 2.39 4.62 Be NO 160020.01-223717.8
16003-2237 LAB 3 2019 198 2 0.2 2.39 4.62 B0.3IV+B2 NO 160020.01-223717.8
16003-2237 LAB 3 2021 201 16 0.1 2.39 4.62 B0.3IV+B2 NO 160020.01-223717.8

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