Abstract
Extensive intermediate band and H..beta.. observations and the available astrometry, have been used to support the suggestions that (1) several southern concentrations of stars are moving with the Pleiades and ..cap alpha.. Persei clusters (Local Association) and (2) the Local Association contains an appreciable percentage of the main-sequence stars near the Sun but the non-random distribution of the brighter association members focuses attention on a few concentrations, or 'clusters'. (3) All of the concentrations discussed here are larger than about 10 pc and the largest, in Lupus-Centaurus, is shown to be accompanied by A to G type main-sequence stars.
Eggen, O J
[1]
- Cerro Tololo Inter-American Observatory, La Serena (Chile)
Citation Formats
Eggen, O J.
Concentrations in the Local Association. 1. The southern concentrations NGC 2516, IC 2602, Centaurus-Lupus and Upper Scorpius.
United Kingdom: N. p.,
1983.
Web.
Eggen, O J.
Concentrations in the Local Association. 1. The southern concentrations NGC 2516, IC 2602, Centaurus-Lupus and Upper Scorpius.
United Kingdom.
Eggen, O J.
1983.
"Concentrations in the Local Association. 1. The southern concentrations NGC 2516, IC 2602, Centaurus-Lupus and Upper Scorpius."
United Kingdom.
@misc{etde_5172562,
title = {Concentrations in the Local Association. 1. The southern concentrations NGC 2516, IC 2602, Centaurus-Lupus and Upper Scorpius}
author = {Eggen, O J}
abstractNote = {Extensive intermediate band and H..beta.. observations and the available astrometry, have been used to support the suggestions that (1) several southern concentrations of stars are moving with the Pleiades and ..cap alpha.. Persei clusters (Local Association) and (2) the Local Association contains an appreciable percentage of the main-sequence stars near the Sun but the non-random distribution of the brighter association members focuses attention on a few concentrations, or 'clusters'. (3) All of the concentrations discussed here are larger than about 10 pc and the largest, in Lupus-Centaurus, is shown to be accompanied by A to G type main-sequence stars.}
journal = []
volume = {204:1}
journal type = {AC}
place = {United Kingdom}
year = {1983}
month = {Jul}
}
title = {Concentrations in the Local Association. 1. The southern concentrations NGC 2516, IC 2602, Centaurus-Lupus and Upper Scorpius}
author = {Eggen, O J}
abstractNote = {Extensive intermediate band and H..beta.. observations and the available astrometry, have been used to support the suggestions that (1) several southern concentrations of stars are moving with the Pleiades and ..cap alpha.. Persei clusters (Local Association) and (2) the Local Association contains an appreciable percentage of the main-sequence stars near the Sun but the non-random distribution of the brighter association members focuses attention on a few concentrations, or 'clusters'. (3) All of the concentrations discussed here are larger than about 10 pc and the largest, in Lupus-Centaurus, is shown to be accompanied by A to G type main-sequence stars.}
journal = []
volume = {204:1}
journal type = {AC}
place = {United Kingdom}
year = {1983}
month = {Jul}
}