The Monitor project: rotation of low-mass stars in the open cluster M34
We report on the results of a V- and i-band time-series photometric survey of M34 (NGC 1039) using the Wide Field Camera (WFC) on the Isaac Newton Telescope (INT), achieving better than 1 per cent precision per data point for 13 ≲i≲ 17. Candidate cluster members were selected from a V versus V−I col...
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| Published in | Monthly notices of the Royal Astronomical Society Vol. 370; no. 2; pp. 954 - 974 |
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| Main Authors | , , , , , , , |
| Format | Journal Article |
| Language | English |
| Published |
Oxford, UK
Blackwell Publishing Ltd
01.08.2006
Oxford University Press Oxford University Press (OUP): Policy P - Oxford Open Option A |
| Subjects | |
| Online Access | Get full text |
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| Abstract | We report on the results of a V- and i-band time-series photometric survey of M34 (NGC 1039) using the Wide Field Camera (WFC) on the Isaac Newton Telescope (INT), achieving better than 1 per cent precision per data point for 13 ≲i≲ 17. Candidate cluster members were selected from a V versus V−I colour-magnitude diagram over 14 < V < 24 (0.12 ≲M/M⊙≲ 1.0), finding 714 candidates, of which we expect ∼400 to be real cluster members (taking into account contamination from the field). The mass function was computed, and found to be consistent with a lognormal distribution in dN/d log M. Searching for periodic variable objects in the candidate members gave 105 detections over the mass range 0.25 < M/M⊙ < 1.0. The distribution of rotation periods for 0.4 < M/M⊙ < 1.0 was found to peak at ∼7 d, with a tail of fast rotators down to periods of ∼0.8 d. For 0.25 < M/M⊙ < 0.4 we found a peak at short periods, with a lack of slow rotators (e.g. P≳ 5 d), consistent with the work of other authors at very low masses. Our results are interpreted in the context of previous work, finding that we reproduce the same general features in the rotational period distributions. A number of rapid rotators were found with velocities ∼ a factor of 2 lower than in the Pleiades, consistent with models of angular momentum evolution assuming solid body rotation without needing to invoke core-envelope decoupling. |
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| AbstractList | We report on the results of a V - and i -band time-series photometric survey of M34 (NGC 1039) using the Wide Field Camera (WFC) on the Isaac Newton Telescope (INT), achieving better than 1 per cent precision per data point for 13 [<, ~]i[<, ~] 17. Candidate cluster members were selected from a V versus V -I colour-magnitude diagram over 14 < V < 24 (0.12 [<, ~]M/M[middot in circle] [<, ~] 1.0), finding 714 candidates, of which we expect ~400 to be real cluster members (taking into account contamination from the field). The mass function was computed, and found to be consistent with a lognormal distribution in dN /d log M . Searching for periodic variable objects in the candidate members gave 105 detections over the mass range 0.25 < M/M[middot in circle] < 1.0. The distribution of rotation periods for 0.4 < M/M[middot in circle] < 1.0 was found to peak at ~7 d, with a tail of fast rotators down to periods of ~0.8 d. For 0.25 < M/M[middot in circle] < 0.4 we found a peak at short periods, with a lack of slow rotators (e.g. P[> ~] 5 d), consistent with the work of other authors at very low masses. Our results are interpreted in the context of previous work, finding that we reproduce the same general features in the rotational period distributions. A number of rapid rotators were found with velocities ~ a factor of 2 lower than in the Pleiades, consistent with models of angular momentum evolution assuming solid body rotation without needing to invoke core-envelope decoupling.[PUBLICATION ABSTRACT] ABSTRACT We report on the results of a V‐ and i‐band time‐series photometric survey of M34 (NGC 1039) using the Wide Field Camera (WFC) on the Isaac Newton Telescope (INT), achieving better than 1 per cent precision per data point for 13 ≲i≲ 17. Candidate cluster members were selected from a V versus V−I colour–magnitude diagram over 14 < V < 24 (0.12 ≲M/M⊙≲ 1.0), finding 714 candidates, of which we expect ∼400 to be real cluster members (taking into account contamination from the field). The mass function was computed, and found to be consistent with a lognormal distribution in dN/d log M. Searching for periodic variable objects in the candidate members gave 105 detections over the mass range 0.25 < M/M⊙ < 1.0. The distribution of rotation periods for 0.4 < M/M⊙ < 1.0 was found to peak at ∼7 d, with a tail of fast rotators down to periods of ∼0.8 d. For 0.25 < M/M⊙ < 0.4 we found a peak at short periods, with a lack of slow rotators (e.g. P≳ 5 d), consistent with the work of other authors at very low masses. Our results are interpreted in the context of previous work, finding that we reproduce the same general features in the rotational period distributions. A number of rapid rotators were found with velocities ∼ a factor of 2 lower than in the Pleiades, consistent with models of angular momentum evolution assuming solid body rotation without needing to invoke core–envelope decoupling. We report on the results of a V- and i-band time-series photometric survey of M34 (NGC 1039) using the Wide Field Camera (WFC) on the Isaac Newton Telescope (INT), achieving better than 1 per cent precision per data point for 13 <~ i <~ 17. Candidate cluster members were selected from a V versus V - I colour-magnitude diagram over 14 < V < 24 (0.12 <~ M/Msolar <~ 1.0), finding 714 candidates, of which we expect ~400 to be real cluster members (taking into account contamination from the field). The mass function was computed, and found to be consistent with a lognormal distribution in dN/d logM. Searching for periodic variable objects in the candidate members gave 105 detections over the mass range 0.25 < M/Msolar < 1.0. The distribution of rotation periods for 0.4 < M/Msolar < 1.0 was found to peak at ~7d, with a tail of fast rotators down to periods of ~0.8d. For 0.25 < M/Msolar < 0.4 we found a peak at short periods, with a lack of slow rotators (e.g. P >~ 5d), consistent with the work of other authors at very low masses. Our results are interpreted in the context of previous work, finding that we reproduce the same general features in the rotational period distributions. A number of rapid rotators were found with velocities ~ a factor of 2 lower than in the Pleiades, consistent with models of angular momentum evolution assuming solid body rotation without needing to invoke core-envelope decoupling. We report on the results of a V- and i-band time-series photometric survey of M34 (NGC 1039) using the Wide Field Camera (WFC) on the Isaac Newton Telescope (INT), achieving better than 1 per cent precision per data point for 13 ≲i≲ 17. Candidate cluster members were selected from a V versus V−I colour-magnitude diagram over 14 < V < 24 (0.12 ≲M/M⊙≲ 1.0), finding 714 candidates, of which we expect ∼400 to be real cluster members (taking into account contamination from the field). The mass function was computed, and found to be consistent with a lognormal distribution in dN/d log M. Searching for periodic variable objects in the candidate members gave 105 detections over the mass range 0.25 < M/M⊙ < 1.0. The distribution of rotation periods for 0.4 < M/M⊙ < 1.0 was found to peak at ∼7 d, with a tail of fast rotators down to periods of ∼0.8 d. For 0.25 < M/M⊙ < 0.4 we found a peak at short periods, with a lack of slow rotators (e.g. P≳ 5 d), consistent with the work of other authors at very low masses. Our results are interpreted in the context of previous work, finding that we reproduce the same general features in the rotational period distributions. A number of rapid rotators were found with velocities ∼ a factor of 2 lower than in the Pleiades, consistent with models of angular momentum evolution assuming solid body rotation without needing to invoke core-envelope decoupling. |
| Author | Hodgkin, Simon Moraux, Estelle Aigrain, Suzanne Irwin, Jonathan Bouvier, Jerome Irwin, Mike Clarke, Cathie Hebb, Leslie |
| Author_xml | – sequence: 1 givenname: Jonathan surname: Irwin fullname: Irwin, Jonathan email: jmi@ast.cam.ac.uk organization: Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA – sequence: 2 givenname: Suzanne surname: Aigrain fullname: Aigrain, Suzanne organization: Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA – sequence: 3 givenname: Simon surname: Hodgkin fullname: Hodgkin, Simon organization: Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA – sequence: 4 givenname: Mike surname: Irwin fullname: Irwin, Mike organization: Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA – sequence: 5 givenname: Jerome surname: Bouvier fullname: Bouvier, Jerome organization: Laboratoire d'Astrophysique, Observatoire de Grenoble, BP 53, F-38041 Grenoble Cédex 9, France – sequence: 6 givenname: Cathie surname: Clarke fullname: Clarke, Cathie organization: Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA – sequence: 7 givenname: Leslie surname: Hebb fullname: Hebb, Leslie organization: School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS – sequence: 8 givenname: Estelle surname: Moraux fullname: Moraux, Estelle organization: Laboratoire d'Astrophysique, Observatoire de Grenoble, BP 53, F-38041 Grenoble Cédex 9, France |
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| SSID | ssj0004326 |
| Score | 2.1459162 |
| Snippet | We report on the results of a V- and i-band time-series photometric survey of M34 (NGC 1039) using the Wide Field Camera (WFC) on the Isaac Newton Telescope... ABSTRACT We report on the results of a V‐ and i‐band time‐series photometric survey of M34 (NGC 1039) using the Wide Field Camera (WFC) on the Isaac Newton... We report on the results of a V - and i -band time-series photometric survey of M34 (NGC 1039) using the Wide Field Camera (WFC) on the Isaac Newton Telescope... |
| SourceID | hal proquest crossref wiley oup istex |
| SourceType | Open Access Repository Aggregation Database Enrichment Source Index Database Publisher |
| StartPage | 954 |
| SubjectTerms | Astronomy open clusters and associations: individual: M34 Sciences of the Universe Stars & galaxies stars: rotation surveys techniques: photometric Time series |
| Title | The Monitor project: rotation of low-mass stars in the open cluster M34 |
| URI | https://api.istex.fr/ark:/67375/WNG-KHZ5T03W-0/fulltext.pdf https://onlinelibrary.wiley.com/doi/abs/10.1111%2Fj.1365-2966.2006.10521.x https://www.proquest.com/docview/207350443 https://hal.science/hal-00398159 |
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