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Title: The Binary Dwarf Carbon Star SDSS J125017.90+252427.6

Journal Article · · The Astrophysical Journal. Letters (Online)

Even though dwarf carbon (dC) stars are universally thought to be binaries in order to explain the presence of C2 in their spectra while still near main-sequence luminosity, direct observational evidence for their binarity is remarkably scarce. In this work, we introduce the detection of a 2.92 day periodicity in both the photometry and radial velocity of SDSS J125017.90+252427.6, an r = 16.4 dC star. This is the first photometric binary dC, and only the second dC spectroscopic binary. The relative phase of the photometric period to the spectroscopic observations suggests that the photometric variations are a reflection effect due to heating from an unseen companion. The observed radial velocity amplitude of the dC component (K = 98.8 ± 10.7 km s-1) is consistent with a white dwarf companion, presumably the evolved star that earlier donated the carbon to the dC, although substantial orbital evolution must have occurred. Large synoptic photometric surveys such as the Palomar Transient Factory, which was used for this work, may prove useful for identifying binaries among the shorter-period dC stars.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE
OSTI ID:
1524173
Journal Information:
The Astrophysical Journal. Letters (Online), Vol. 856, Issue 1; ISSN 2041-8213
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 9 works
Citation information provided by
Web of Science

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Cited By (8)

The GALAH survey: a catalogue of carbon-enhanced stars and CEMP candidates journal November 2018
Distances of Dwarf Carbon Stars journal May 2018
The Time-domain Spectroscopic Survey: Radial Velocity Variability in Dwarf Carbon Stars journal May 2019
A Chandra Study: Are Dwarf Carbon Stars Spun Up and Rejuvenated by Mass Transfer? journal August 2019
Wolf 1465: Not a Bright Dwarf Carbon Star journal April 2018
Distances of Dwarf Carbon Stars text January 2018
Wolf 1465: Not a Bright Dwarf Carbon Star text January 2018
A Chandra Study: Are Dwarf Carbon Stars Spun Up and Rejuvenated by Mass Transfer? text January 2019

Figures / Tables (4)


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