Diagramas Hertzsprung-Russell de cúmulos estelares en la Vía Láctea a partir de Gaia Data Release 3

"Una de las formas de estudiar la Vía Láctea es mediante el análisis de diagramas Hertzsprung-Russell, que permiten el estudio de estrellas según su ubicación en los mismos. Los cúmulos estelares son un ejemplo de este tipo de estudios. Tales objetos son estructuras formadas por muchas estrella...

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Autores:
Medina Botero, María Angélica
Tipo de recurso:
Trabajo de grado de pregrado
Fecha de publicación:
2023
Institución:
Universidad de los Andes
Repositorio:
Séneca: repositorio Uniandes
Idioma:
spa
OAI Identifier:
oai:repositorio.uniandes.edu.co:1992/69088
Acceso en línea:
http://hdl.handle.net/1992/69088
Palabra clave:
Gaia DR3
Cúmulos estelares
Vía Láctea
Diagramas Hertzsprung-Russell
Física
Rights
openAccess
License
https://repositorio.uniandes.edu.co/static/pdf/aceptacion_uso_es.pdf
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repository_id_str
dc.title.none.fl_str_mv Diagramas Hertzsprung-Russell de cúmulos estelares en la Vía Láctea a partir de Gaia Data Release 3
title Diagramas Hertzsprung-Russell de cúmulos estelares en la Vía Láctea a partir de Gaia Data Release 3
spellingShingle Diagramas Hertzsprung-Russell de cúmulos estelares en la Vía Láctea a partir de Gaia Data Release 3
Gaia DR3
Cúmulos estelares
Vía Láctea
Diagramas Hertzsprung-Russell
Física
title_short Diagramas Hertzsprung-Russell de cúmulos estelares en la Vía Láctea a partir de Gaia Data Release 3
title_full Diagramas Hertzsprung-Russell de cúmulos estelares en la Vía Láctea a partir de Gaia Data Release 3
title_fullStr Diagramas Hertzsprung-Russell de cúmulos estelares en la Vía Láctea a partir de Gaia Data Release 3
title_full_unstemmed Diagramas Hertzsprung-Russell de cúmulos estelares en la Vía Láctea a partir de Gaia Data Release 3
title_sort Diagramas Hertzsprung-Russell de cúmulos estelares en la Vía Láctea a partir de Gaia Data Release 3
dc.creator.fl_str_mv Medina Botero, María Angélica
dc.contributor.advisor.none.fl_str_mv Sabogal Martínez, Beatriz Eugenia
dc.contributor.author.none.fl_str_mv Medina Botero, María Angélica
dc.contributor.jury.none.fl_str_mv García Varela, José Alejandro
dc.contributor.researchgroup.es_CO.fl_str_mv Grupo de astronomía
dc.subject.keyword.none.fl_str_mv Gaia DR3
Cúmulos estelares
Vía Láctea
Diagramas Hertzsprung-Russell
topic Gaia DR3
Cúmulos estelares
Vía Láctea
Diagramas Hertzsprung-Russell
Física
dc.subject.themes.es_CO.fl_str_mv Física
description "Una de las formas de estudiar la Vía Láctea es mediante el análisis de diagramas Hertzsprung-Russell, que permiten el estudio de estrellas según su ubicación en los mismos. Los cúmulos estelares son un ejemplo de este tipo de estudios. Tales objetos son estructuras formadas por muchas estrellas que están ligadas entre sí debido a la gravedad y que tienen un origen común. Al ubicar estos cúmulos en el diagrama HR, es posible entender la evolución de la galaxia en la que se encuentran. En este proyecto se construyeron múltiples diagramas Hertzsprung-Russell para, a partir de la ubicación de las estrellas de cada cúmulo, analizar sus etapas evolutivas. A la vez, se llevó esto a cabo buscando actualizar el diagrama de Sandage (1958), ampliamente usado en la astronomía, por lo cual se usaron los mismos cúmulos implementados por este, junto con otros nueve cúmulos más." -Tomado del documento de grado
publishDate 2023
dc.date.accessioned.none.fl_str_mv 2023-08-02T18:29:58Z
dc.date.available.none.fl_str_mv 2023-08-02T18:29:58Z
dc.date.issued.none.fl_str_mv 2023-06-01
dc.type.es_CO.fl_str_mv Trabajo de grado - Pregrado
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dc.relation.references.es_CO.fl_str_mv Babusiaux C., et al., 2018, Gaia Data Release 2-Observational Hertzsprung-Russell diagrams, Astronomy & Astrophysics, 616, A10
Alfonso J. E., et al., 2019, Pertenencia de estrellas a cúmulos abiertos usando movimientos propios de Gaia. Uniandes.
Bessell M. S., 2005, Standard photometric systems, Annu. Rev. Astron. Astrophys., 43, 293
Carroll B. W., Ostlie D. A., 2017, An introduction to modern astrophysics. Cambridge University Press
Collaboration G., et al., 2018, Summary of the contents and survey properties, Astronomy and Astrophysics, 616, A1
ESA 2022a, GAIA DATA RELEASE 3, https://www.cosmos.esa.int/web/gaia/dr3
ESA 2022b, Technical report, The Gaia mission. European Space Agency
ESA 2023, HIPPARCOS HERTZSPRUNG-RUSSELL DIAGRAMS, https://www.cosmos.esa.int/web/hipparcos/h-r-diagrams
ESA/Hubble 2021b, Technical report, Image Archive: Star Clusters, https://esahubble .org/images/archive/category/starclusters/. ESA/Hubble, https://esahubble .org/images/archive/category/starclusters/
ESA/Hubble 2021a, Technical report, Open Cluster, https://esahubble.org/wordbank/ open-cluster/. ESA/Hubble, https://esahubble.org/wordbank/open-cluster/
Evans D., Riello M., De Angeli F., Carrasco J., Montegriffo P., et al., 2018, Gaia data release 2-photometric content and validation, Astronomy & Astrophysics, 616, A4
Ferraro F., Paltrinieri B., Pecci F. F., Cacciari C., Dorman B., et al., 1997, HST observations of blue straggler stars in the core of the globular cluster M3, arXiv preprint astroph/9703026
Friel E., 1995, The old open clusters of the Milky Way, Annual Review of Astronomy and Astrophysics, 33, 381
Hansen C. J., Kawaler S. D., Trimble V., 2012, Stellar interiors: physical principles, structure, and evolution. Springer Science & Business Media
Heber U., 2009, Hot subdwarf stars, Annual review of Astronomy and Astrophysics, 47, 211
Johnson H., 1963, Photometric Systems. the University of Chicago Press
Jordi C., Gebran M., Carrasco J., De Bruijne J., Voss H., et al., 2010, Gaia broad band photometry, Astronomy & Astrophysics, 523, A48
Karttunen H., Kröger P., Oja H., Poutanen M., Donner K. J., 2007, Fundamental astronomy. Springer
Kerber F., Mignani R., Guglielmetti F., Wicenec A., 2003, Galactic Planetary Nebulae and their central stars-I. An accurate and homogeneous set of coordinates, Astronomy & Astrophysics, 408, 1029
Krumholz M. R., McKee C. F., Bland-Hawthorn J., 2019, Star clusters across cosmic time, Annual Review of Astronomy and Astrophysics, 57, 227
Kwok S., Purton C. R., Fitzgerald P. M., 1978, On the origin of planetary nebulae, The Astrophysical Journal, 219, L125
Lada C. J., Lada E. A., 2003, Embedded clusters in molecular clouds, Annual Review of Astronomy and Astrophysics, 41, 57
Langer N., Kudritzki R., 2014, The spectroscopic Hertzsprung-Russell diagram, Astronomy & Astrophysics, 564, A52
Minniti D., Navarro M. G., 2019, The VVV Survey: Globular Clusters and more, Proceedings of the International Astronomical Union, 14, 31¿34
Mucciarelli A., Dalessandro E., Massari D., Bellazzini M., Ferraro F. R., et al., 2016, NGC 6362: the least massive globular cluster with chemically distinct multiple populations, The Astrophysical Journal, 824, 73
Murdin P., 2001, Encyclopedia of Astronomy & Astrophysics. CRC Press
Pols O. R., 2011, Stellar structure and evolution. Astronomical Institute Utrecht NY
Prialnik D., 2000, An introduction to the theory of stellar structure and evolution. Cambridge University Press
Prusti T., De Bruijne J., Brown A. G., Vallenari A., Babusiaux C., et al., 2016, The gaia mission, Astronomy & astrophysics, 595, A1
Rich R. M., Sosin C., Djorgovski S. G., Piotto G., King I. R., et al., 1997, Discovery of extended blue horizontal branches in two metal-rich globular clusters, The Astrophysical Journal, 484, L25
Riello M., De Angeli F., Evans D., Montegriffo P., Carrasco J., et al., 2021, Gaia early data release 3-photometric content and validation, Astronomy & Astrophysics, 649, A3
Rowell N., Davidson M., Lindegren L., Van Leeuwen F., Castañeda J., et al., 2021, Gaia Early Data Release 3-Modelling and calibration of Gaia¿s point and line spread functions, Astronomy & Astrophysics, 649, A11
Russell H. N., 1979, 35. Relations between the Spectra and Other Characteristics of Stars. Harvard University Press, Cambridge, MA and London, England, pp 212¿ 220, doi:doi:10.4159/harvard.9780674366688.c39, https://doi.org/10.4159/harvard .9780674366688.c39
Salaris M., Cassisi S., 2005, Evolution of stars and stellar populations. John Wiley & Sons
Sandage A. R., 1953, The color-magnitude diagram for the globular cluster M3., The Astronomical Journal, 58, 61
Sandage A., 1958, The color-magnitude diagrams of galactic and globular clusters and their interpretation as age groups, Ricerche Astronomiche, 5, 41
Spitzer L., Shull J. M., 1975, Random gravitational encounters and the evolution of spherical systems. VII-Systems with several mass groups, The Astrophysical Journal, 201, 773
Stanek K., Mateo M., Udalski A., Szymanski M., Kaluzny J., et al., 1994, Color-Magnitude Diagram Distribution of the Bulge Red Clump Stars-Evidence for the Galactic Bar, arXiv preprint astro-ph/9404026
Strand K. A., 1977, in The HR Diagram, In Memory of Henry Norris Russell. IAU Symposium No. 80, held November 2, 1977, at the National Academy of Sciences, Washington, DC. Report No. 13, edited by AG Davis Philip and David H. DeVorkin, December, 1977., p. 55. p. 55
Van Leeuwen F., Vallenari A., Jordi C., Lindegren L., Bastian U., et al., 2017, Gaia Data Release 1-Open cluster astrometry: performance, limitations, and future prospects, Astronomy & Astrophysics, 601, A19
Vasiliev E., 2019, Proper motions and dynamics of the Milky Way globular cluster system from Gaia DR2, Monthly Notices of the Royal Astronomical Society, 484, 2832
Wang P., Chen W., Lin C., Pandey A., Huang C., et al., 2014, Characterization of the Praesepe star cluster by photometry and proper motions with 2MASS, PPMXL, and PanSTARRS, The Astrophysical Journal, 784, 57
Wenger M., Ochsenbein F., Egret D., Dubois P., Bonnarel F., et al., 2000, The SIMBAD astronomical database-The CDS reference database for astronomical objects, Astronomy and Astrophysics Supplement Series, 143, 9
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spelling Sabogal Martínez, Beatriz Eugenia4952c2bf-83fd-4933-bed4-1403477529b5600Medina Botero, María Angélicaa91cc4c5-c356-4c89-8eb4-42ef3a92cee6600García Varela, José AlejandroGrupo de astronomía2023-08-02T18:29:58Z2023-08-02T18:29:58Z2023-06-01http://hdl.handle.net/1992/69088instname:Universidad de los Andesreponame:Repositorio Institucional Sénecarepourl:https://repositorio.uniandes.edu.co/"Una de las formas de estudiar la Vía Láctea es mediante el análisis de diagramas Hertzsprung-Russell, que permiten el estudio de estrellas según su ubicación en los mismos. Los cúmulos estelares son un ejemplo de este tipo de estudios. Tales objetos son estructuras formadas por muchas estrellas que están ligadas entre sí debido a la gravedad y que tienen un origen común. Al ubicar estos cúmulos en el diagrama HR, es posible entender la evolución de la galaxia en la que se encuentran. En este proyecto se construyeron múltiples diagramas Hertzsprung-Russell para, a partir de la ubicación de las estrellas de cada cúmulo, analizar sus etapas evolutivas. A la vez, se llevó esto a cabo buscando actualizar el diagrama de Sandage (1958), ampliamente usado en la astronomía, por lo cual se usaron los mismos cúmulos implementados por este, junto con otros nueve cúmulos más." -Tomado del documento de gradoFísicoPregradoAstronomía62 páginasapplication/pdfspaUniversidad de los AndesFísicaFacultad de CienciasDepartamento de Físicahttps://repositorio.uniandes.edu.co/static/pdf/aceptacion_uso_es.pdfinfo:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Diagramas Hertzsprung-Russell de cúmulos estelares en la Vía Láctea a partir de Gaia Data Release 3Trabajo de grado - Pregradoinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_7a1fTexthttp://purl.org/redcol/resource_type/TPGaia DR3Cúmulos estelaresVía LácteaDiagramas Hertzsprung-RussellFísicahttps://doi.org/10.5270/esa-qa4lep3Babusiaux C., et al., 2018, Gaia Data Release 2-Observational Hertzsprung-Russell diagrams, Astronomy & Astrophysics, 616, A10Alfonso J. E., et al., 2019, Pertenencia de estrellas a cúmulos abiertos usando movimientos propios de Gaia. Uniandes.Bessell M. S., 2005, Standard photometric systems, Annu. Rev. Astron. Astrophys., 43, 293Carroll B. W., Ostlie D. A., 2017, An introduction to modern astrophysics. Cambridge University PressCollaboration G., et al., 2018, Summary of the contents and survey properties, Astronomy and Astrophysics, 616, A1ESA 2022a, GAIA DATA RELEASE 3, https://www.cosmos.esa.int/web/gaia/dr3ESA 2022b, Technical report, The Gaia mission. European Space AgencyESA 2023, HIPPARCOS HERTZSPRUNG-RUSSELL DIAGRAMS, https://www.cosmos.esa.int/web/hipparcos/h-r-diagramsESA/Hubble 2021b, Technical report, Image Archive: Star Clusters, https://esahubble .org/images/archive/category/starclusters/. ESA/Hubble, https://esahubble .org/images/archive/category/starclusters/ESA/Hubble 2021a, Technical report, Open Cluster, https://esahubble.org/wordbank/ open-cluster/. ESA/Hubble, https://esahubble.org/wordbank/open-cluster/Evans D., Riello M., De Angeli F., Carrasco J., Montegriffo P., et al., 2018, Gaia data release 2-photometric content and validation, Astronomy & Astrophysics, 616, A4Ferraro F., Paltrinieri B., Pecci F. F., Cacciari C., Dorman B., et al., 1997, HST observations of blue straggler stars in the core of the globular cluster M3, arXiv preprint astroph/9703026Friel E., 1995, The old open clusters of the Milky Way, Annual Review of Astronomy and Astrophysics, 33, 381Hansen C. J., Kawaler S. D., Trimble V., 2012, Stellar interiors: physical principles, structure, and evolution. Springer Science & Business MediaHeber U., 2009, Hot subdwarf stars, Annual review of Astronomy and Astrophysics, 47, 211Johnson H., 1963, Photometric Systems. the University of Chicago PressJordi C., Gebran M., Carrasco J., De Bruijne J., Voss H., et al., 2010, Gaia broad band photometry, Astronomy & Astrophysics, 523, A48Karttunen H., Kröger P., Oja H., Poutanen M., Donner K. J., 2007, Fundamental astronomy. SpringerKerber F., Mignani R., Guglielmetti F., Wicenec A., 2003, Galactic Planetary Nebulae and their central stars-I. An accurate and homogeneous set of coordinates, Astronomy & Astrophysics, 408, 1029Krumholz M. R., McKee C. F., Bland-Hawthorn J., 2019, Star clusters across cosmic time, Annual Review of Astronomy and Astrophysics, 57, 227Kwok S., Purton C. R., Fitzgerald P. M., 1978, On the origin of planetary nebulae, The Astrophysical Journal, 219, L125Lada C. J., Lada E. A., 2003, Embedded clusters in molecular clouds, Annual Review of Astronomy and Astrophysics, 41, 57Langer N., Kudritzki R., 2014, The spectroscopic Hertzsprung-Russell diagram, Astronomy & Astrophysics, 564, A52Minniti D., Navarro M. G., 2019, The VVV Survey: Globular Clusters and more, Proceedings of the International Astronomical Union, 14, 31¿34Mucciarelli A., Dalessandro E., Massari D., Bellazzini M., Ferraro F. R., et al., 2016, NGC 6362: the least massive globular cluster with chemically distinct multiple populations, The Astrophysical Journal, 824, 73Murdin P., 2001, Encyclopedia of Astronomy & Astrophysics. CRC PressPols O. R., 2011, Stellar structure and evolution. Astronomical Institute Utrecht NYPrialnik D., 2000, An introduction to the theory of stellar structure and evolution. Cambridge University PressPrusti T., De Bruijne J., Brown A. G., Vallenari A., Babusiaux C., et al., 2016, The gaia mission, Astronomy & astrophysics, 595, A1Rich R. M., Sosin C., Djorgovski S. G., Piotto G., King I. R., et al., 1997, Discovery of extended blue horizontal branches in two metal-rich globular clusters, The Astrophysical Journal, 484, L25Riello M., De Angeli F., Evans D., Montegriffo P., Carrasco J., et al., 2021, Gaia early data release 3-photometric content and validation, Astronomy & Astrophysics, 649, A3Rowell N., Davidson M., Lindegren L., Van Leeuwen F., Castañeda J., et al., 2021, Gaia Early Data Release 3-Modelling and calibration of Gaia¿s point and line spread functions, Astronomy & Astrophysics, 649, A11Russell H. N., 1979, 35. Relations between the Spectra and Other Characteristics of Stars. Harvard University Press, Cambridge, MA and London, England, pp 212¿ 220, doi:doi:10.4159/harvard.9780674366688.c39, https://doi.org/10.4159/harvard .9780674366688.c39Salaris M., Cassisi S., 2005, Evolution of stars and stellar populations. John Wiley & SonsSandage A. R., 1953, The color-magnitude diagram for the globular cluster M3., The Astronomical Journal, 58, 61Sandage A., 1958, The color-magnitude diagrams of galactic and globular clusters and their interpretation as age groups, Ricerche Astronomiche, 5, 41Spitzer L., Shull J. M., 1975, Random gravitational encounters and the evolution of spherical systems. VII-Systems with several mass groups, The Astrophysical Journal, 201, 773Stanek K., Mateo M., Udalski A., Szymanski M., Kaluzny J., et al., 1994, Color-Magnitude Diagram Distribution of the Bulge Red Clump Stars-Evidence for the Galactic Bar, arXiv preprint astro-ph/9404026Strand K. A., 1977, in The HR Diagram, In Memory of Henry Norris Russell. IAU Symposium No. 80, held November 2, 1977, at the National Academy of Sciences, Washington, DC. Report No. 13, edited by AG Davis Philip and David H. DeVorkin, December, 1977., p. 55. p. 55Van Leeuwen F., Vallenari A., Jordi C., Lindegren L., Bastian U., et al., 2017, Gaia Data Release 1-Open cluster astrometry: performance, limitations, and future prospects, Astronomy & Astrophysics, 601, A19Vasiliev E., 2019, Proper motions and dynamics of the Milky Way globular cluster system from Gaia DR2, Monthly Notices of the Royal Astronomical Society, 484, 2832Wang P., Chen W., Lin C., Pandey A., Huang C., et al., 2014, Characterization of the Praesepe star cluster by photometry and proper motions with 2MASS, PPMXL, and PanSTARRS, The Astrophysical Journal, 784, 57Wenger M., Ochsenbein F., Egret D., Dubois P., Bonnarel F., et al., 2000, The SIMBAD astronomical database-The CDS reference database for astronomical objects, Astronomy and Astrophysics Supplement Series, 143, 9201814201PublicationTHUMBNAILDiagramas_Hertzsprung_Russell_GDR3.pdf.jpgDiagramas_Hertzsprung_Russell_GDR3.pdf.jpgIM Thumbnailimage/jpeg7394https://repositorio.uniandes.edu.co/bitstreams/44d4ac9c-8568-4597-8780-c2a9f43cc397/download5c619388474f6294516a423f6746b213MD55autorizacion.pdf.jpgautorizacion.pdf.jpgIM Thumbnailimage/jpeg18724https://repositorio.uniandes.edu.co/bitstreams/8e138f2e-2e01-4794-8005-c83509c709fb/download8e54668d4fb02be6e40bddcfda14f095MD57LICENSElicense.txtlicense.txttext/plain; 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