J/A+A/417/961       UBV(RI)c photometry of NGC 2580 and NGC 2588  (Baume+, 2004)

NGC 2580 and NGC 2588. Two open clusters in the Third Galactic Quadrant. Baume G., Moitinho A., Giorgi E.E., Carraro G., Vazquez R.A. <Astron. Astrophys., 417, 961-972 (2004)> =2004A&A...417..961B 2004A&A...417..961B
ADC_Keywords: Clusters, open ; Photometry, UBVRI Keywords: Galaxy: open clusters and associations: general - Galaxy: open clusters and associations: individual: NGC 2580, NGC 2588 Abstract: We present CCD broad band photometric observations in the fields of the Third Galactic Quadrant open clusters NGC 2580 and NGC 2588 (V(I)c and UBV(RI)c respectively). From the analysis of our data we found that NGC 2580 is located at a distance of about 4kpc and its age is close to 160Myr. As for NGC 2588, it is placed at about 5kpc from the Sun and is 450Myr old. This means that NGC 2588 belongs to the extension of the Perseus arm, whereas NGC 2580 is closer to the local arm structure. The luminosity functions (LFs) have been constructed for both clusters down to V∼20 together with their initial mass functions (IMFs) for stars with masses above M∼1-1.5M. The IMF slopes for the most massive bins yielded values of x∼1.3 for NGC 2580 and x∼2 for NGC 2588. In the case of this latter cluster we found evidence of a core-corona structure produced probably by dynamical effect. In the main sequences of both clusters we detected gaps, which we suggest could be real features. Description: Our data set comes from CCD photometric observations carried out in the course of several runs on different telescopes: - The European Southern Observatory (ESO): CCD VI observations of the fields of NGC 2580 and NGC 2588 using the new EMMI read arm camera at the NTT in the photometric night of December 9, 2002. - The Complejo Astronomico El Leoncito (CASLEO): In the night January 25, 1996 CCD UBV observations of NGC 2588 were performed using the 215cm telescope. - The Cerro Tololo Inter-American Observatory (CTIO): UBV(RI)c CCD photometric data of the field of NGC 2588 were acquired with the 0.9m telescope on the night of January 1, 1998. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3a.dat 114 3171 Photometric catalogue of the NGC 2580 region table3b.dat 156 4306 Photometric catalogue of the NGC 2588 region -------------------------------------------------------------------------------- See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) I/259 : The Tycho-2 Catalogue (Hog+ 2000) Byte-by-byte Description of file: table3a.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 5- 8 I4 --- Seq Identification number (this work) 12- 17 F6.1 pix Xpos X position in arcseconds (1) 21- 26 F6.1 pix Ypos Y position in arcseconds (1) 29- 30 I2 h RAh Right Ascension (J2000) 32- 33 I2 min RAm Right Ascension (J2000) 35- 38 F4.1 s RAs Right Ascension (J2000) 41 A1 --- DE- Declination sign (J2000) 42- 43 I2 deg DEd Declination (J2000) 45- 46 I2 arcmin DEm Declination (J2000) 48- 51 F4.1 arcsec DEs Declination (J2000) 56- 60 F5.2 mag Vmag V magnitude 62- 63 A2 --- u_Vmag Comments for V magnitude (G1) 68- 72 F5.2 mag V-Ic ? V-Ic colour index 74- 75 A2 --- u_V-Ic Comments for V-Ic index (G1) 77- 78 A2 --- Memb Membership assignment (G2) 81- 96 A16 --- 2MASS 2MASS designation (JHHMMSSss-DDMMSS) 98 A1 --- --- [=] 100-102 A3 --- --- [TYC] 104-115 A12 --- TYC TYCHO-2 identification (TYC FFFF-NNNNN-N) -------------------------------------------------------------------------------- Note (1): Adopted center: NGC 2580: 08:21:28.0-30:18:00.0 (J2000) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3b.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 5- 8 I4 --- Seq Identification number (this work) 12- 17 F6.1 pix Xpos X position in arcseconds (1) 21- 26 F6.1 pix Ypos Y position in arcseconds (1) 29- 30 I2 h RAh Right Ascension (J2000) 32- 33 I2 min RAm Right Ascension (J2000) 35- 38 F4.1 s RAs Right Ascension (J2000) 41 A1 --- DE- Declination sign (J2000) 42- 43 I2 deg DEd Declination (J2000) 45- 46 I2 arcmin DEm Declination (J2000) 48- 51 F4.1 arcsec DEs Declination (J2000) 56- 60 F5.2 mag Vmag V magnitude 62- 63 A2 --- u_Vmag Comments for V magnitude (G1) 68- 72 F5.2 mag B-V ? B-Vc colour index 74- 75 A2 --- u_B-V Comments for B-V index (G1) 80- 84 F5.2 mag U-B ? U-Bc colour index 86- 87 A2 --- u_U-B Comments for U-B index (G1) 92- 96 F5.2 mag V-Rc ? V-Rc colour index 98- 99 A2 --- u_V-Rc Comments for V-Rc index (G1) 105-109 F5.2 mag V-Ic ? V-Ic colour index 111-112 A2 --- u_V-Ic Comments for V-Ic index (G1) 114-121 A8 --- Memb Membership assignment (G2) (2) 123-138 A16 --- 2MASS 2MASS designation (JHHMMSSss-DDMMSS) 140 A1 --- --- [=] 142-144 A3 --- --- [TYC] 146-157 A12 --- TYC TYCHO-2 identification (TYC FFFF-NNNNN-N) -------------------------------------------------------------------------------- Note (1): Adopted center: NGC 2588: 08:23:10.0-32:58:30.0 (J2000) Note (2): Additional membership assignment for NGC 2588 pm(red) = probable member in the red clump pm(bin?) = probable member and probable binary star nm(fgr) = nom-member: foreground star -------------------------------------------------------------------------------- Globla notes: Note (G1): Comments on photometry: (: ) error larger than 0.05 (::) error larger than 0.10 Note (G2): Membership assignment: lm = likely member pm = probable member nm = non-member -------------------------------------------------------------------------------- Acknowledgements: Gustavo L. Baume
(End) Patricia Bauer [CDS] 24-May-2004
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line