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Topic: IC 2602

	Abstract of ESO Scientific Preprint No 1211 (Site not responding. Last check: 2007-11-06)
		G and early-K IC 2602 stars are, on average, somewhat more Li-rich than their counterparts in the two slightly older clusters.
		Finally, the latest-type IC 2602 stars are heavily Li depleted, with their Li content being as low as the lowest measured among the Pleiades.
		As in the Pleiades and Alpha Per, a star-to-star scatter in lithium is observed among 30 Myr old late-K/early-K dwarfs in IC 2602, indicating that this spread develops in the pre--main sequence phases.
	www.eso.org /gen-fac/pubs/bin/prep-abs-sci/science-pp-1997.txt/1211 (183 words)

	Canberra Astronomical Society - Southern Cross - April 2000
		The large open cluster IC 2602 (RA 10h 43m, Dec -64 24'), for example, centred on the star Theta Carinae, is too big for the telescope and needs the wider field of view that binoculars provide.
		IC 2714 (11h 18m, -62 42') is located less than a degree to the north.
		IC 2501 (9h 39m, -60 05'), a stellar planetary nebula, needed the OIII filter to identify it by blocking out the nearby stars.
	msowww.anu.edu.au /cas/southerncross/sc_200004.html (2228 words)

	The Evolution of Rotation and Activity in Young Open Clusters: The Zero--Age Main Sequence (Site not responding. Last check: 2007-11-06)
		With cluster ages of 30-50 Myr, IC 2391 and IC 2602 are ideal laboratories in which to observe conditions at the ZAMS since the solar-type stars in these clusters have not been on the main sequence long enough to undergo significant magnetic braking.
		Among the IC 2391 and IC 2602 K dwarfs, we observe a factor of $\sim$10 spread in the distribution of rotation periods.
		When compared to data from clusters like the Pleiades and the Hyades, we find there are stars in IC 2391 and IC 2602 with rotation rates and activity levels similar to those observed in the older clusters.
	www.aas.org /publications/baas/v26n4/aas185/abs/S9801.html (345 words)

	[No title]
		1994 have been plotted.}}{13}} \@writefile{toc}{\string\contentsline\space {subsubsection}{\string\numberline\space {4.1.2.}Late-type stars: Comparison to the Pleiades}{13}} \@writefile{lof}{\string\contentsline\space {figure}{\string\numberline\space {5}{\ignorespaces {\string\pbf\space a)} Logarithm of X-ray luminosities as a function of B$-$V color for good photometric IC 2602 candidates (objects indicated with ``Y" and ``Y?" in Tab.
		The position of R95B is explicitly indicated in the figure (see text).}}{14}} \@writefile{lof}{\string\contentsline\space {figure}{\string\numberline\space {7}{\ignorespaces X-ray luminosity as a function of $B - V$ color for the present IC 2602 sample (filled squares), the Pleiades from Stauffer et al.
		(1994; open circles), and IC 2391 objects from Patten \& Simon (1993; open squares).}}{15}} \@writefile{lot}{\string\contentsline\space {table}{\string\numberline\space {5}{\ignorespaces Comparison of the mean and median X-ray luminosity}}{15}} \@writefile{lof}{\string\contentsline\space {figure}{\string\numberline\space {8}{\ignorespaces {\string\pbf\space a)} Cumulative X-ray luminosity distribution functions for IC 2602 candidates (solid curve) and Pleiades objects from Stauffer et al.
	cfa-www.harvard.edu /~stauffer/wwwpapers/ic2602.aux (286 words)

	IC 2602 (Site not responding. Last check: 2007-11-06)
		Open Cluster IC 2602 (= Lacaille II.9 = Melotte 102 = Collinder 229), in Carina
		The splendid open cluster IC 2602 was discovered by Abbe Lacaille on March 3, 1752 from South Africa, and cataloged as Lacaille II.9.
		The distance of IC 2602 has been slightly adjusted from the data of the Hipparcos satellite; according to these data, the cluster is at 479 light years (the older value had been 489 light years).
	www.seds.org /messier/xtra/ngc/i2602.html (174 words)

	Trans Global (Site not responding. Last check: 2007-11-06)
		Date: Mon, 28 Jul 1997 23:23:03 PDT Former IC GP26's 2601 and 2602 and SD28 9450 departed Council Bluffs, IA July 29 on train CBBI-29, dead in tow and destined for Trans Global Rail in Des Moines, IA. Also in train was former IC GP10 8170, destined for National Railway in Silvis, IL.
		As stated in Allan's note, IC 2602, 2601 and 9450 had been moved to the rebuilding facility.
		Both 2602 and 2601 have Alco trucks under an EMD carbody.
	www.simpson.edu /~tinder/080397DesMoines/080397DesMoines.html (426 words)

	SCYON: Paper abstracts (Site not responding. Last check: 2007-11-06)
		We studied the fields of nine nearby open star clusters based on the Tycho-2 catalogue.
		The clusters are: Blanco 1, Stock 2, the alpha Per cluster, the Pleiades, NGC 2451, IC 2391, Praesepe, IC 2602, and NGC 7092.
		We determined membership probabilities for the stars in the cluster fields from the stellar proper motions and used the Tycho-2 photometry to compute the initial mass function (IMF) of the clusters from the main sequence turn-off point down to approx.
	obswww.unige.ch /webda/scyon/Sanner_1.html (193 words)

	Catalogue: J/A+A/372/862/stars (Site not responding. Last check: 2007-11-06)
		J/A+A/372/862 Lithium abundances in IC 2602 and IC 2391 (Randich+, 2001) ================================================================================ Membership, lithium, and metallicity in the young open clusters IC 2602 and IC 2391: enlarging the sample Randich S., Pallavicini R., Meola G., Stauffer J.R., Balachandran S.C.
		372, 862 (2001)> =2001A&A...372..862R ================================================================================ ADC_Keywords: Clusters, open ; Abundances, peculiar Keywords: open clusters and associations: individual: IC 2602, IC 2391 - stars: abundances - stars: interiors Description: Lithium abundances and [Fe/H] for a sample of late-type stars in the young open clusters IC 2602 and IC 2391.
		Note (1): Star designations: IC 2602 RNNA = [RSP95] NNNA IC 2602 WNNN = Cl* IC 2602 W NNN IC 2391 VXRNNA = VXR PSPC NNa IC 2391 SHJM NN = Cl* IC 2391 SHJM NN Note (2): Asterisks indicate stars for which errors in Teff could not be directly estimated
	vizier.u-strasbg.fr /cgi-bin/Cat?J/A+A/372/862/stars (541 words)

	Other open clusters observed by Hipparcos (Site not responding. Last check: 2007-11-06)
		1997); on Praesepe, IC 4756, NGC 6475, NGC 6633, Stock 2, NGC 2516 and NGC 3532 (Robichon et al.
		The mean distances of all these clusters have been determined from Hipparcos intermediate data of member stars, taking into account the correlations between the abscissae of stars within a few degrees of the sky (such as in clusters) due to the operation mode of the satellite.
		The Pleiades, and probably IC 2391 and IC 2602, define a sequence about 0.5 mag fainter that the previous one (Mermilliod et al.
	astro.u-strasbg.fr /howfar/turon/node6.html (398 words)

	[No title] (Site not responding. Last check: 2007-11-06)
		We present the results of ROSAT PSPC observations of the 30 Myr old IC 2602 cluster; for the X-ray detected objects the results of a CCD photometric survey are also given.
		We construct X-ray luminosity distribution functions for objects in different color ranges and we compare them with those for the Pleiades.
		F, G, and early--K type candidates in IC 2602 appear to be more X-ray luminous than in the Pleiades, while no significant difference is seen among late--K and M dwarfs.
	cfa-www.harvard.edu /~stauffer/wwwpapers/ic2602.abstract.html (225 words)

	CCD photometry of late-type stars in the young open cluster IC 2602 (Site not responding. Last check: 2007-11-06)
		CCD photometry of late-type stars in the young open cluster IC 2602
		We present the results of VRI photometry of the young open cluster IC 2602.
		Two 15x15arcmin^2^ fields were observed in February and May 1991 using the 1-m Swope telescope at Las Campanas.
	www.cs.wisc.edu /niagara/data/nasa/A+AS_126_81.xml (158 words)

	Departamento de Astrofísica (UCM), Cúmulos Abiertos Jovenes / Young Open Clusters (Site not responding. Last check: 2007-11-06)
		(3) "Rotational Velocities and Chromospheric/Coronal Activity of Low-Mass Stars in the Young Open Clusters IC 2391 and IC 2602", Stauffer J.R., et al.
		(6) "Membership, lithium, and metallicity in the young open clusters IC 2602 and IC 2391: enlarging the sample", Randich et al., 2001, A&A, in press
		(8) "Membership, lithium, and metallicity in the young open clusters IC 2602 and IC 2391: enlarging the sample", Randich et al., 2001, A&A, 372, 862
	www.ucm.es /info/Astrof/invest/actividad/cumulos.html (3224 words)

	Auckland Astronomical Society
		Easily seen from dark skies and outlying suburbs well away from the hub of the inner city, a treasure trove of celestial “jewels” awaits the anticipating eye.
		Here we can explore the playground of the “rich and famous”; dazzling open clusters such as IC 2602, the “Southern Pleiades” and the glorious NGC 3532.
		Nearby lies the expansive eta Carinae nebula, seeded with the light of many clusters and laced with dark lanes of dust.
	www.astronomy.org.nz /aas/Journal/NightOfTheStars.asp (1140 words)

	(IAAC) Obj: IC 2602 (theta Car, Southern Pleiades) - Inst: 10x50 handhel (Site not responding. Last check: 2007-11-06)
		Subject: (IAAC) Obj: IC 2602 (theta Car, Southern Pleiades) - Inst: 10x50 handheld binoculars
		Class: II 3 m Constellation: Car Data: mag 1.9 size 50' Position: RA 10:43 DEC -64:23 Description: IC 2602 is the southernmost of the three bright clusters that surround Eta Carina.
		I believe that it is only because of its low altitude that I cannot see it naked eye.
	www.visualdeepsky.org /netastrocatalog/msg00596.html (168 words)

	DOC: Uranometria chart 449
		It is recorded in the IC as "planetary, stellar, 10.5 mag." The nebula measures 6 arcseconds across and Vorontsov-Velyaminov describes it as stellar.
		Hartung writes: "This is a good example of a 'stellar' planetary nebula, only to be distinguished from the starry field by the single prism image, though with care a minute bluish disk can be made out.
		Nice contrast with IC 2714, which lies to the north in the same low-power field.
	www.fortunecity.com /roswell/borley/49/u449.htm (2881 words)

	Giuseppina Micela (Site not responding. Last check: 2007-11-06)
		PATTEN B.M. and SIMON T. The evolution of rotation and activity in young open clusters: IC 2391, 1996, ApJS, 106, 489-532
		PATTEN B.M. The evolution of rotation and activity in young open clusters: the zero-age main sequence, 1994, BAAS, 26, 1478
		PATTEN B.M. and SIMON T., A ROSAT PSPC observation of the young cluster IC 2391, 1993, BAAS, 25, 883
	www.astropa.unipa.it /~giusi/OCLUSTER/ic2391.refX.html (136 words)

	(IAAC) Obj: IC 2391 (omicron Vel) - Inst: naked eye, 10x50 handheld bino (Site not responding. Last check: 2007-11-06)
		Class: II 2 p Constellation: Vel Data: mag 2.5 size 50' Position: RA 08:40 DEC -53:00 Description: IC 2391 is on the west side of the False Cross.
		Naked eye visible as a dim patch with two stars involved.
		Next: (IAAC) Obj: IC 2602 (theta Car, Southern Pleiades) - Inst: 10x50 handheld binoculars
	www.visualdeepsky.org /netastrocatalog/msg00597.html (136 words)

	Constellation Carina
		Open clusters: NGC 2516, NGC 3114, NGC 3293, NGC 3532, IC 2602, I 2714, Mel 105
		One of the more famous is IC 2602, sometimes called the Southern Pleiades.
		The name is derived from the Argo Navis, the ship of the Argonauts, of which Carina, the keel, is thought to be a part of.
	www.maa.mhn.de /Maps/Stars_en/Fig/carina.html (638 words)

	[No title]
		GCh,RW Privatdancer Johnny M. "Be Good," 04-10-1992, Champagne Mink, 2602-794598, IC= _________
		Ginjon's Taffetta Cremepuff, 07-23-1984, Platinum Solid, 2699-223700, IC= 28.12500
		Toytown's Kiss Me Kate of Selkatz, 12-20-1998, Champagne Mink, 2608-1067312, IC= 10.81183
	selkatztonkinese.com /pedigreehannah.html (257 words)

	WEBDA: Database contents
		A photometric and spectroscopic search for white dwarfs in the young open cluster IC 2602
		A study of the galactic cluster IC 2602.
		A new approach to Zero-Age main sequence fitting
	www.univie.ac.at /webda/cgi-bin/detail.cgi?ubvpe+ic2602 (118 words)

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