A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397
- Autores
- Pichardo Marcano, Manuel; Rivera Sandoval, Liliana E.; Maccarone, Thomas J.; Rohrmann, Rene Daniel; Althaus, Leandro Gabriel; Heinke, Craig O.; Belloni, Diogo; Bahramian, Arash
- Año de publicación
- 2025
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Using archival Hubble Space Telescope observations, we report the discovery of four variable low-mass white dwarfs (WDs; 0.18 M⊙ ≤ M ≤ 0.5 M⊙) in the globular cluster NGC 6397. One source exhibits a periodic optical modulation of 5.21 ± 0.02 hr, which we interpret as potentially due to the rotation of a magnetic helium core WD (He WD). This makes this candidate the second magnetic He WD in NGC 6397, and one of the few He WDs with a measured rotation period. The other three candidates show aperiodic variability, with a change in magnitude ranging from ∼0.11 to 0.6. These discoveries highlight the importance of high-cadence photometric surveys in dense stellar environments. Follow-up spectroscopic observations are needed to confirm the nature of the variability of these systems.
Fil: Pichardo Marcano, Manuel. University of Texas at Austin; Estados Unidos
Fil: Rivera Sandoval, Liliana E.. University of Texas at Austin; Estados Unidos
Fil: Maccarone, Thomas J.. University of Texas at Austin; Estados Unidos
Fil: Rohrmann, Rene Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Heinke, Craig O.. University of Texas at Austin; Estados Unidos
Fil: Belloni, Diogo. University of Texas at Austin; Estados Unidos
Fil: Bahramian, Arash. University of Texas at Austin; Estados Unidos - Materia
- white dwarf
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
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- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/290791
Ver los metadatos del registro completo
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A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397Pichardo Marcano, ManuelRivera Sandoval, Liliana E.Maccarone, Thomas J.Rohrmann, Rene DanielAlthaus, Leandro GabrielHeinke, Craig O.Belloni, DiogoBahramian, Arashwhite dwarfhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Using archival Hubble Space Telescope observations, we report the discovery of four variable low-mass white dwarfs (WDs; 0.18 M⊙ ≤ M ≤ 0.5 M⊙) in the globular cluster NGC 6397. One source exhibits a periodic optical modulation of 5.21 ± 0.02 hr, which we interpret as potentially due to the rotation of a magnetic helium core WD (He WD). This makes this candidate the second magnetic He WD in NGC 6397, and one of the few He WDs with a measured rotation period. The other three candidates show aperiodic variability, with a change in magnitude ranging from ∼0.11 to 0.6. These discoveries highlight the importance of high-cadence photometric surveys in dense stellar environments. Follow-up spectroscopic observations are needed to confirm the nature of the variability of these systems.Fil: Pichardo Marcano, Manuel. University of Texas at Austin; Estados UnidosFil: Rivera Sandoval, Liliana E.. University of Texas at Austin; Estados UnidosFil: Maccarone, Thomas J.. University of Texas at Austin; Estados UnidosFil: Rohrmann, Rene Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; ArgentinaFil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Heinke, Craig O.. University of Texas at Austin; Estados UnidosFil: Belloni, Diogo. University of Texas at Austin; Estados UnidosFil: Bahramian, Arash. University of Texas at Austin; Estados UnidosIOP Publishing2025-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/290791Pichardo Marcano, Manuel; Rivera Sandoval, Liliana E.; Maccarone, Thomas J.; Rohrmann, Rene Daniel; Althaus, Leandro Gabriel; et al.; A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397; IOP Publishing; Astrophysical Journal; 979; 2; 1-2025; 1-100004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ada144info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ada144info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-08-25T15:45:15Zoai:ri.conicet.gov.ar:11336/290791instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982026-08-25 15:45:16.577CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397 |
| title |
A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397 |
| spellingShingle |
A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397 Pichardo Marcano, Manuel white dwarf |
| title_short |
A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397 |
| title_full |
A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397 |
| title_fullStr |
A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397 |
| title_full_unstemmed |
A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397 |
| title_sort |
A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397 |
| dc.creator.none.fl_str_mv |
Pichardo Marcano, Manuel Rivera Sandoval, Liliana E. Maccarone, Thomas J. Rohrmann, Rene Daniel Althaus, Leandro Gabriel Heinke, Craig O. Belloni, Diogo Bahramian, Arash |
| author |
Pichardo Marcano, Manuel |
| author_facet |
Pichardo Marcano, Manuel Rivera Sandoval, Liliana E. Maccarone, Thomas J. Rohrmann, Rene Daniel Althaus, Leandro Gabriel Heinke, Craig O. Belloni, Diogo Bahramian, Arash |
| author_role |
author |
| author2 |
Rivera Sandoval, Liliana E. Maccarone, Thomas J. Rohrmann, Rene Daniel Althaus, Leandro Gabriel Heinke, Craig O. Belloni, Diogo Bahramian, Arash |
| author2_role |
author author author author author author author |
| dc.subject.none.fl_str_mv |
white dwarf |
| topic |
white dwarf |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Using archival Hubble Space Telescope observations, we report the discovery of four variable low-mass white dwarfs (WDs; 0.18 M⊙ ≤ M ≤ 0.5 M⊙) in the globular cluster NGC 6397. One source exhibits a periodic optical modulation of 5.21 ± 0.02 hr, which we interpret as potentially due to the rotation of a magnetic helium core WD (He WD). This makes this candidate the second magnetic He WD in NGC 6397, and one of the few He WDs with a measured rotation period. The other three candidates show aperiodic variability, with a change in magnitude ranging from ∼0.11 to 0.6. These discoveries highlight the importance of high-cadence photometric surveys in dense stellar environments. Follow-up spectroscopic observations are needed to confirm the nature of the variability of these systems. Fil: Pichardo Marcano, Manuel. University of Texas at Austin; Estados Unidos Fil: Rivera Sandoval, Liliana E.. University of Texas at Austin; Estados Unidos Fil: Maccarone, Thomas J.. University of Texas at Austin; Estados Unidos Fil: Rohrmann, Rene Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Heinke, Craig O.. University of Texas at Austin; Estados Unidos Fil: Belloni, Diogo. University of Texas at Austin; Estados Unidos Fil: Bahramian, Arash. University of Texas at Austin; Estados Unidos |
| description |
Using archival Hubble Space Telescope observations, we report the discovery of four variable low-mass white dwarfs (WDs; 0.18 M⊙ ≤ M ≤ 0.5 M⊙) in the globular cluster NGC 6397. One source exhibits a periodic optical modulation of 5.21 ± 0.02 hr, which we interpret as potentially due to the rotation of a magnetic helium core WD (He WD). This makes this candidate the second magnetic He WD in NGC 6397, and one of the few He WDs with a measured rotation period. The other three candidates show aperiodic variability, with a change in magnitude ranging from ∼0.11 to 0.6. These discoveries highlight the importance of high-cadence photometric surveys in dense stellar environments. Follow-up spectroscopic observations are needed to confirm the nature of the variability of these systems. |
| publishDate |
2025 |
| dc.date.none.fl_str_mv |
2025-01 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/290791 Pichardo Marcano, Manuel; Rivera Sandoval, Liliana E.; Maccarone, Thomas J.; Rohrmann, Rene Daniel; Althaus, Leandro Gabriel; et al.; A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397; IOP Publishing; Astrophysical Journal; 979; 2; 1-2025; 1-10 0004-637X CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/290791 |
| identifier_str_mv |
Pichardo Marcano, Manuel; Rivera Sandoval, Liliana E.; Maccarone, Thomas J.; Rohrmann, Rene Daniel; Althaus, Leandro Gabriel; et al.; A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397; IOP Publishing; Astrophysical Journal; 979; 2; 1-2025; 1-10 0004-637X CONICET Digital CONICET |
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eng |
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eng |
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IOP Publishing |
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IOP Publishing |
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