A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397

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 rota...

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Main Authors: Manuel Pichardo Marcano, Liliana E. Rivera Sandoval, Thomas J. Maccarone, Rene D. Rohrmann, Leandro G. Althaus, Craig O. Heinke, Diogo Belloni, Arash Bahramian
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/ada144
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author Manuel Pichardo Marcano
Liliana E. Rivera Sandoval
Thomas J. Maccarone
Rene D. Rohrmann
Leandro G. Althaus
Craig O. Heinke
Diogo Belloni
Arash Bahramian
author_facet Manuel Pichardo Marcano
Liliana E. Rivera Sandoval
Thomas J. Maccarone
Rene D. Rohrmann
Leandro G. Althaus
Craig O. Heinke
Diogo Belloni
Arash Bahramian
author_sort Manuel Pichardo Marcano
collection DOAJ
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.
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spelling doaj-art-ed680348ff0d47dea4a0d8e3e48fbfb22025-01-24T10:03:37ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01979216710.3847/1538-4357/ada144A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397Manuel Pichardo Marcano0https://orcid.org/0000-0003-4436-831XLiliana E. Rivera Sandoval1https://orcid.org/0000-0002-9396-7215Thomas J. Maccarone2https://orcid.org/0000-0003-0976-4755Rene D. Rohrmann3https://orcid.org/0000-0001-7209-3574Leandro G. Althaus4https://orcid.org/0000-0003-2771-7805Craig O. Heinke5https://orcid.org/0000-0003-3944-6109Diogo Belloni6https://orcid.org/0000-0003-1535-0866Arash Bahramian7https://orcid.org/0000-0003-2506-6041Department of Life and Physical Sciences, Fisk University , 1000 17th Avenue N., Nashville, TN 37208, USA ; mmarcano@fisk.edu; Department of Physics and Astronomy, Vanderbilt University , 6301 Stevenson Center Lane, Nashville, TN 37235, USADepartment of Physics and Astronomy, University of Texas Rio Grande Valley , Brownsville, TX 78520, USADepartment of Physics and Astronomy, Texas Tech University , Lubbock, TX 79409, USAInstituto de Ciencias Astronómicas , de la Tierra y del Espacio (CONICET-UNSJ), Av. España 1512 (sur), 5400 San Juan, ArgentinaGrupo de Evolución Estelar y Pulsaciones. Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata , Paseo del Bosque s/n, 1900 La Plata, Argentina; IALP—CONICET , La Plata, ArgentinaDepartment of Physics, University of Alberta , CCIS 4-183, Edmonton, AB, T6G 2E1, CanadaDepartamento de Física, Universidad Técnica Federico Santa María , Av. España 1680, Valparaíso, ChileInternational Center for Radio Astronomy Research Curtin University , GPO Box U1987, Perth, WA 6845, AustraliaUsing 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.https://doi.org/10.3847/1538-4357/ada144White dwarf starsGlobular star clustersStellar magnetic fields
spellingShingle Manuel Pichardo Marcano
Liliana E. Rivera Sandoval
Thomas J. Maccarone
Rene D. Rohrmann
Leandro G. Althaus
Craig O. Heinke
Diogo Belloni
Arash Bahramian
A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397
The Astrophysical Journal
White dwarf stars
Globular star clusters
Stellar magnetic fields
title 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_short A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397
title_sort second candidate magnetic helium core white dwarf and 3 other variable white dwarfs in the globular cluster ngc 6397
topic White dwarf stars
Globular star clusters
Stellar magnetic fields
url https://doi.org/10.3847/1538-4357/ada144
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