He+He white dwarf SDSS J232230.20+050942.0 RVels Virtual Observatory Resource

Authors
  1. Brown W.R.
  2. Kilic M.
  3. Bedard A.
  4. Kosakowski A.
  5. Bergeron P.
  6. Published by
    CDS
Abstract

We report the discovery of a 1201s orbital period binary, the third shortest-period detached binary known. Sloan Digital Sky Survey J232230.20+050942.06 contains two He-core white dwarfs orbiting with a 27{deg} inclination. Located 0.76kpc from the Sun, the binary has an estimated Laser Interferometer Space Antenna (LISA) 4yr signal-to-noise ratio of 40. J2322+0509 is the first He+He white dwarf LISA verification binary, a source class that is predicted to account for one-third of resolved LISA ultra-compact binary detections.

Keywords
  1. spectroscopic-binary-stars
  2. white-dwarf-stars
  3. radial-velocity
  4. visible-astronomy
Bibliographic source Bibcode
2020ApJ...892L..35B
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/892/L35
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/892/L35
Document Object Identifer DOI
doi:10.26093/cds/vizier.18929035

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/892/L35
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/892/L35
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/892/L35
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2021-09-16T12:23:22Z
Resource record created
2021-09-16T12:23:22Z
Created
2022-09-13T11:37:04Z
Updated

Contact

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CDS support team
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