Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/33121
DC Field | Value | Language |
---|---|---|
dc.contributor.author | BEDIN, Luigi | en_US |
dc.contributor.author | Salaris, M. | en_US |
dc.contributor.author | Anderson, J. | en_US |
dc.contributor.author | Libralato, M. | en_US |
dc.contributor.author | Apai, D. | en_US |
dc.contributor.author | Nardiello, D. | en_US |
dc.contributor.author | Rich, R. M. | en_US |
dc.contributor.author | Bellini, A. | en_US |
dc.contributor.author | Dieball, A. | en_US |
dc.contributor.author | Bergeron, P. | en_US |
dc.contributor.author | Burgasser, A. J. | en_US |
dc.contributor.author | Milone, A. P. | en_US |
dc.contributor.author | Marino, A. F. | en_US |
dc.date.accessioned | 2023-02-02T13:00:43Z | - |
dc.date.available | 2023-02-02T13:00:43Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/33121 | - |
dc.description.abstract | We report on the white dwarf (WD) cooling sequence of the old globular cluster NGC 6752, which is chemically complex and hosts a blue horizontal branch. This is one of the last globular cluster WD cooling sequences accessible to imaging by the Hubble Space Telescope. Our photometry and completeness tests show that we have reached the peak of the luminosity function of the WD cooling sequence, at a magnitude m<SUB>F606W</SUB> = 29.4 ± 0.1, which is consistent with a formal age of ∼14 Gyr. This age is also consistent with the age from fits to the main-sequence turn-off (13-14 Gyr), reinforcing our conclusion that we observe the expected accumulation of WDs along the cooling sequence. | en_US |
dc.language.iso | eng | en_US |
dc.title | The HST large programme on NGC 6752 - III. Detection of the peak of the white dwarf luminosity function | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stz1968 | en_US |
dc.identifier.scopus | 2-s2.0-85082569332 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/488/3/3857/5533339 | en_US |
dc.identifier.url | http://arxiv.org/abs/1907.06300v1 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 488 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 3857 | en_US |
dc.relation.lastpage | 3865 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019MNRAS.488.3857B | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairetype | Article | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0003-4080-6466 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
stz1968.pdf | Pdf editoriale | 3.76 MB | Adobe PDF | View/Open |
Items in DSpace are published in Open Access, unless otherwise indicated.