Zwicky Transient Facility and Globular Clusters: The Period–Luminosity and Period–Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud Sample

We present the first gri -band period–luminosity (PL) and period–Wesenheit (PW) relations for the fundamental mode anomalous Cepheids. These PL and PW relations were derived from a combined sample of five anomalous Cepheids in globular cluster M92 and the Large Magellanic Cloud, both of which have d...

Full description

Bibliographic Details
Main Authors: Chow-Choong Ngeow, Anupam Bhardwaj, Matthew J. Graham, Steven L. Groom, Frank J. Masci, Reed Riddle
Format: Article
Language:English
Published: IOP Publishing 2022-01-01
Series:The Astronomical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-3881/ac8df2
_version_ 1827827592074362880
author Chow-Choong Ngeow
Anupam Bhardwaj
Matthew J. Graham
Steven L. Groom
Frank J. Masci
Reed Riddle
author_facet Chow-Choong Ngeow
Anupam Bhardwaj
Matthew J. Graham
Steven L. Groom
Frank J. Masci
Reed Riddle
author_sort Chow-Choong Ngeow
collection DOAJ
description We present the first gri -band period–luminosity (PL) and period–Wesenheit (PW) relations for the fundamental mode anomalous Cepheids. These PL and PW relations were derived from a combined sample of five anomalous Cepheids in globular cluster M92 and the Large Magellanic Cloud, both of which have distance accurate to ∼1% available from literature. Our g -band PL relation is similar to the B -band PL relation as reported in previous study. We applied our PL and PW relations to anomalous Cepheids discovered in dwarf galaxy Crater II, and found a larger but consistent distance modulus than the recent measurements based on RR Lyrae. Our calibrations of gri -band PL and PW relations, even though less precise due to small number of anomalous Cepheids, will be useful for distance measurements to dwarf galaxies.
first_indexed 2024-03-12T03:35:17Z
format Article
id doaj.art-fa85f68b4f34493dbc969c6694bafd4b
institution Directory Open Access Journal
issn 1538-3881
language English
last_indexed 2024-03-12T03:35:17Z
publishDate 2022-01-01
publisher IOP Publishing
record_format Article
series The Astronomical Journal
spelling doaj.art-fa85f68b4f34493dbc969c6694bafd4b2023-09-03T13:19:57ZengIOP PublishingThe Astronomical Journal1538-38812022-01-01164519110.3847/1538-3881/ac8df2Zwicky Transient Facility and Globular Clusters: The Period–Luminosity and Period–Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud SampleChow-Choong Ngeow0https://orcid.org/0000-0001-8771-7554Anupam Bhardwaj1https://orcid.org/0000-0001-6147-3360Matthew J. Graham2https://orcid.org/0000-0002-3168-0139Steven L. Groom3https://orcid.org/0000-0001-5668-3507Frank J. Masci4https://orcid.org/0000-0002-8532-9395Reed Riddle5https://orcid.org/0000-0002-0387-370XGraduate Institute of Astronomy, National Central University , 300 Jhongda Road, 32001 Jhongli, Taiwan ; cngeow@astro.ncu.edu.twINAF-Osservatorio astronomico di Capodimonte , Via Moiariello 16, I-80131 Napoli, ItalyDivision of Physics, Mathematics, and Astronomy, California Institute of Technology , Pasadena, CA 91125, USAIPAC, California Institute of Technology , 1200 E. California Boulevard, Pasadena, CA 91125, USAIPAC, California Institute of Technology , 1200 E. California Boulevard, Pasadena, CA 91125, USACaltech Optical Observatories, California Institute of Technology , Pasadena, CA 91125, USAWe present the first gri -band period–luminosity (PL) and period–Wesenheit (PW) relations for the fundamental mode anomalous Cepheids. These PL and PW relations were derived from a combined sample of five anomalous Cepheids in globular cluster M92 and the Large Magellanic Cloud, both of which have distance accurate to ∼1% available from literature. Our g -band PL relation is similar to the B -band PL relation as reported in previous study. We applied our PL and PW relations to anomalous Cepheids discovered in dwarf galaxy Crater II, and found a larger but consistent distance modulus than the recent measurements based on RR Lyrae. Our calibrations of gri -band PL and PW relations, even though less precise due to small number of anomalous Cepheids, will be useful for distance measurements to dwarf galaxies.https://doi.org/10.3847/1538-3881/ac8df2Globular star clustersAnomalous Cepheid variable starsSky surveysDistance indicators
spellingShingle Chow-Choong Ngeow
Anupam Bhardwaj
Matthew J. Graham
Steven L. Groom
Frank J. Masci
Reed Riddle
Zwicky Transient Facility and Globular Clusters: The Period–Luminosity and Period–Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud Sample
The Astronomical Journal
Globular star clusters
Anomalous Cepheid variable stars
Sky surveys
Distance indicators
title Zwicky Transient Facility and Globular Clusters: The Period–Luminosity and Period–Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud Sample
title_full Zwicky Transient Facility and Globular Clusters: The Period–Luminosity and Period–Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud Sample
title_fullStr Zwicky Transient Facility and Globular Clusters: The Period–Luminosity and Period–Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud Sample
title_full_unstemmed Zwicky Transient Facility and Globular Clusters: The Period–Luminosity and Period–Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud Sample
title_short Zwicky Transient Facility and Globular Clusters: The Period–Luminosity and Period–Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud Sample
title_sort zwicky transient facility and globular clusters the period luminosity and period wesenheit relations for anomalous cepheids supplemented with large magellanic cloud sample
topic Globular star clusters
Anomalous Cepheid variable stars
Sky surveys
Distance indicators
url https://doi.org/10.3847/1538-3881/ac8df2
work_keys_str_mv AT chowchoongngeow zwickytransientfacilityandglobularclusterstheperiodluminosityandperiodwesenheitrelationsforanomalouscepheidssupplementedwithlargemagellaniccloudsample
AT anupambhardwaj zwickytransientfacilityandglobularclusterstheperiodluminosityandperiodwesenheitrelationsforanomalouscepheidssupplementedwithlargemagellaniccloudsample
AT matthewjgraham zwickytransientfacilityandglobularclusterstheperiodluminosityandperiodwesenheitrelationsforanomalouscepheidssupplementedwithlargemagellaniccloudsample
AT stevenlgroom zwickytransientfacilityandglobularclusterstheperiodluminosityandperiodwesenheitrelationsforanomalouscepheidssupplementedwithlargemagellaniccloudsample
AT frankjmasci zwickytransientfacilityandglobularclusterstheperiodluminosityandperiodwesenheitrelationsforanomalouscepheidssupplementedwithlargemagellaniccloudsample
AT reedriddle zwickytransientfacilityandglobularclusterstheperiodluminosityandperiodwesenheitrelationsforanomalouscepheidssupplementedwithlargemagellaniccloudsample