| dc.contributor |
Jordi i Nebot, Carme |
|
| dc.contributor |
Masana Fresno, Eduard |
|
| dc.contributor |
Balaguer Núñez, María de los Dolores |
|
| dc.creator |
Massana Zapata, Pol |
|
| dc.date |
2016-10-26T13:41:01Z |
|
| dc.date |
2016-10-26T13:41:01Z |
|
| dc.date |
2016-06 |
|
| dc.date.accessioned |
2024-12-16T10:23:20Z |
|
| dc.date.available |
2024-12-16T10:23:20Z |
|
| dc.identifier |
http://hdl.handle.net/2445/102934 |
|
| dc.identifier.uri |
http://fima-docencia.ub.edu:8080/xmlui/handle/123456789/15836 |
|
| dc.description |
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutors: Carme Jordi Nebot, Eduard Masana Fresno, Lola Balaguer Núñez |
|
| dc.description |
In this study a characterisation of the physical parameters of the open cluster M67 is
made by using empirical calibrations in the Ströomgren-Crawford filter system. A group of 316 stars
contributed to the results. The photometric analysis leads to an extinction of Eb-y = 0:03 +- 0:03,
a distance modulus V0 - Mv = 9:6 +- 0:3 (or 830 +- 60 pc), a metallicity [Fe=H] = 0:0 +- 0:3 and the
age of the cluster is approximated to be log t(yr) = 9:57 +- 0:05 (or 3:72 +- 0:19 Gyr) |
|
| dc.format |
5 p. |
|
| dc.format |
application/pdf |
|
| dc.language |
eng |
|
| dc.rights |
cc-by-nc-nd (c) Massana, 2016 |
|
| dc.rights |
http://creativecommons.org/licenses/by-nc-nd/3.0/es/ |
|
| dc.rights |
info:eu-repo/semantics/openAccess |
|
| dc.source |
Treballs Finals de Grau (TFG) - Física |
|
| dc.subject |
Cúmuls d'estels |
|
| dc.subject |
Fotometria astronòmica |
|
| dc.subject |
Treballs de fi de grau |
|
| dc.subject |
Clusters of stars |
|
| dc.subject |
Astronomical photometry |
|
| dc.subject |
Bachelor's theses |
|
| dc.title |
Characterisation of the open cluster M67 |
|
| dc.type |
info:eu-repo/semantics/bachelorThesis |
|