دورية أكاديمية
Ground-based CCD astrometry with wide-field imagers - II. A star catalog for m 67: WFI@2.2 m MPG/ESO astrometry, FLAMES @ VLT radial velocities
| العنوان: | Ground-based CCD astrometry with wide-field imagers - II. A star catalog for m 67: WFI@2.2 m MPG/ESO astrometry, FLAMES @ VLT radial velocities |
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| المؤلفون: | YADAV RKS, ANDERSON J, CASSISI S, PLATAIS I, PASQUINI L, SAGAR R., BEDIN, LUIGI, PIOTTO, GIAMPAOLO, VILLANOVA, SANDRO, AL MOMANY, YAZAN |
| المساهمون: | Yadav, Rk, Bedin, Luigi, Piotto, Giampaolo, Anderson, J, Cassisi, S, Villanova, Sandro, Platais, I, Pasquini, L, AL MOMANY, Yazan, Sagar, R. |
| سنة النشر: | 2008 |
| المجموعة: | Padua Research Archive (IRIS - Università degli Studi di Padova) |
| الوصف: | Context: The solar-age open cluster M 67 (C0847+120, NGC 2682) is a touchstone in studies of the old Galactic disk. Despite its outstanding role, the census of cluster membership for M 67 at fainter magnitudes and their properties are not well-established. Aims: Using proprietary and archival ESO data, we have obtained astrometric, photometric, and radial velocities of stars in a 34×33 arcmin2 field centered on the old open cluster M 67. Methods: The two-epoch archival observations separated by 4 years and acquired with the Wide-Field Imager at the 2.2 m MPG/ESO telescope were reduced with our new astrometric techniques, as described in the first paper in this series. The same observations served to derive calibrated BVI photometry in M 67. Radial velocities were measured using the archival and new spectroscopic data obtained at the VLT. Results: We have determined relative proper motions and membership probabilities for ~2400 stars. The precision of proper motions for optimally exposed stars is 1.9 mas yr-1, gradually degrading down to ~5 mas yr-1 at V=20. Our relatively precise proper motions at V>16 were first obtained in this magnitude range for M 67. Radial velocities were measured for 211 stars in the same field. We also present a detailed comparison with recent theoretical isochrones from several independent groups. Conclusions: For the M 67 area, we provide positions, calibrated BVI photometry, relative proper motions, membership probabilities, and radial velocities. We demonstrate that ground-based CCD mosaic observations just a few years apart are producing proper motions, allowing reliable membership determination. We have produced a catalog that is electronically available to the astronomical community. Based on observations with the MPG/ESO 2.2 m and ESO/VLT telescopes, located at La Silla and Paranal Observatory, Chile, under DDT program 278.D-5027, and the archive material. This is paper 33 of the WIYN Open Cluster Study (WOCS). Full Table [see full text] is only available in electronic form at ... |
| نوع الوثيقة: | article in journal/newspaper |
| اللغة: | English |
| العلاقة: | info:eu-repo/semantics/altIdentifier/wos/WOS:000256309700039; volume:484; firstpage:609; lastpage:620; journal:ASTRONOMY & ASTROPHYSICS; http://hdl.handle.net/11577/2268905Test; info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-44449179204 |
| DOI: | 10.1051/0004-6361:20079245 |
| الإتاحة: | https://doi.org/10.1051/0004-6361:20079245Test http://hdl.handle.net/11577/2268905Test |
| رقم الانضمام: | edsbas.DDE3014F |
| قاعدة البيانات: | BASE |
| DOI: | 10.1051/0004-6361:20079245 |
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