1978
DOI: 10.1093/mnras/182.4.607
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NGC 6383 - I. The central core

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Cited by 16 publications
(44 citation statements)
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“…Our results are in reasonable agreement with the upper age limit of 4 Myr inferred by Paunzen et al (2007). We note that FitzGerald et al (1978) derived a younger cluster age of 1.7 ± 0.4 Myr. The difference may originate from the use of different PMS isochrones or the work of FitzGerald et al (1978) being restricted to the brighter cluster members only.…”
Section: The Hertzsprung-russell Diagramsupporting
confidence: 92%
See 1 more Smart Citation
“…Our results are in reasonable agreement with the upper age limit of 4 Myr inferred by Paunzen et al (2007). We note that FitzGerald et al (1978) derived a younger cluster age of 1.7 ± 0.4 Myr. The difference may originate from the use of different PMS isochrones or the work of FitzGerald et al (1978) being restricted to the brighter cluster members only.…”
Section: The Hertzsprung-russell Diagramsupporting
confidence: 92%
“…The last column yields the cross identification with objects previously studied by FitzGerald et al (1978) as well as some information about objects with Hα emission. JHK photometric system of Bessell & Brett (1988).…”
Section: Near Infrared Photometrymentioning
confidence: 99%
“…The cluster HR diagram is very well defined and the derived cluster age, ∼ 3 Myr, agrees with the most of the values found in the literature (Fitzgerald et al 1978;Battinelli & CapuzzoDolcetta 1991;Kharchenko et al 2005;Paunzen et al 2007 (see Fig. 6, second more bright star of the sample) and accept that the X-Ray Be binary star No.…”
Section: Ngc 6383supporting
confidence: 90%
“…Three young clusters are found within a projected radius of 65 pc, among which NGC 6383 belonging to Sgr OB1 association with an estimated age of 1.7 Myr. NGC 6383 is at 1.5 kpc from the Sun (Fitzgerald et al 1978), comparable to HD 158186's distance.…”
Section: Hd 158186mentioning
confidence: 86%