2003ApJ...595.1124M


Query : 2003ApJ...595.1124M

2003ApJ...595.1124M - Astrophys. J., 595, 1124-1130 (2003/October-1)

The massive triple star system HD 16429 A.

McSWAIN M.V.

Abstract (from CDS):

HD 16429 A is a triple star system consisting of a single-lined spectroscopic binary and a widely separated third component, previously identified via speckle interferometry. Here I present the first orbital elements for the unblended spectroscopic binary as well as estimates of the spectral types and relative flux contributions for each visible component based on a Doppler tomographic reconstruction of their spectra. There are several stars around HD 16429 A, including the nearby Be X-ray binary and microquasar LS I +61°303, which all probably belong to a subcluster within the Cas OB6 association.

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Journal keyword(s): Stars: Binaries: Spectroscopic - Stars: Early-Type - Stars: Individual: Henry Draper Number: HD 16429

Simbad objects: 9

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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 LS I +61 303 HXB 02 40 31.6644419688 +61 13 45.593918580 11.27 11.61 10.75 10.19 9.55 B0Ve 903 2
2 AG+61 253 * 02 40 44.7754371168 +61 16 49.428608844   10.29 9.83     F5V 10 0
3 HD 16429 ** 02 40 44.9492589168 +61 16 55.995618720 7.91 8.29 7.67     O9.5III+F4V 165 1
4 BD+60 542 * 02 40 46.1369674104 +61 17 48.508997748   11.14 10.44     O9-B0IV-V 17 0
5 LS I +61 306 * 02 40 51.0471822888 +61 15 45.446713272   11.52 11.10     O9.5-B0IV-V 14 0
6 Ass Cas OB 6 As* 02 43 +61.3           ~ 128 0
7 V* AE Aur Or* 05 16 18.1493304816 +34 18 44.344404000 5.48 6.18 5.96     O9.5V 597 1
8 * 15 Mon Be* 06 40 58.65963 +09 53 44.7229 3.360 4.45 4.68   4.88 O7V+B1.5/2V 823 0
9 * zet Aql PM* 19 05 24.6080155 +13 51 48.518212 2.99 3.00 2.99 2.98 2.98 A0IV-Vnn 364 0

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