Cl* NGC 133 C 13 , the SIMBAD biblio

2002A&A...387..479C - Astronomy and Astrophysics, volume 387, 479-486 (2002/5-4)

A photometric study of the two poorly known northern open clusters NGC 133 and NGC 1348.

CARRARO G.

Abstract (from CDS):

We present CCD UBVI observations obtained in the field of the previously unstudied northern open clusters NGC 133 and NGC 1348. We argue that NGC 133 is a heavily contaminated cluster, for which we identify 13 candidate members down to V=14.50mag on the basis of the position in the two-color Diagram. Membership has been checked against proper motions from Tycho 2, whenever available. The cluster turns out to have a reddening E(B-V)=0.60±0.10mag, to be 630±150pc distant from the Sun, and to have an age less than 10Myrs. NGC 1348 is a more reddened clusters (E(B-V)=0.85±0.15mag) for which we isolate 20 members. The cluster lies at a distance of 1.9±0.5kpc away from the Sun, and has an age greater than 50Myrs.

Abstract Copyright:

Journal keyword(s): open clusters and associations: individual: NGC 133, NGC 1348 - open clusters and associations: general

VizieR on-line data: <Available at CDS (J/A+A/387/479): ngc133.dat ngc1348.dat>

Nomenclature: ngc133.dat: Cl* NGC 133 C NNN N=309 among (Nos 1-347). ngc1348.dat: Cl* NGC 1348 C NNN N=141 among (Nos 1-147).

Status at CDS:   All or part of tables of objects will not be ingested in SIMBAD.

CDS comments: In table 3 : positions of ID1 are positions of TYC 4019 744 1(ID2). C 0 028+60 is a misprint for 0028+630.

Simbad objects: 17

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2020.08.03-23:34:42

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