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Ultra-short period compact binaries are important sources of gravitational waves, which include e.g. the progenitors of type Ia supernovae or the progenitors of merger episodes that may lead to massive and magnetic single white dwarfs.…

We report the detection of the likely companion of the binary millisecond pulsar J0740+6620 with the Gran Telescopio Canarias in the $r'$ and $i'$ bands. The position of the detected starlike source coincides with the pulsar coordinates…

Solar and Stellar Astrophysics · Physics 2019-03-04 D. M. Beronya , A. V. Karpova , A. Yu. Kirichenko , S. V. Zharikov , D. A. Zyuzin , Yu. A. Shibanov , A. Cabrera-Lavers

The aim of the Degenerate Objects around Degenerate Objects (DODO) survey is to search for very low mass brown dwarfs and extrasolar planets in wide orbits around white dwarfs via direct imaging. The direct detection of such companions…

Earth and Planetary Astrophysics · Physics 2011-03-17 E. Hogan , M. R. Burleigh , F. J. Clarke

We have identified eight to ten new cool white dwarfs from the Large Area Survey (LAS) Data Release 9 of the United Kingdom InfraRed Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS). The data set was paired with the Sloan Digital Sky…

Solar and Stellar Astrophysics · Physics 2014-05-02 P. -E. Tremblay , S. K. Leggett , N. Lodieu , B. Freytag , P. Bergeron , J. S. Kalirai , H. -G. Ludwig

We present infrared H- and K-band spectra of a companion candidate 3" north of the young star GSC 08047-00232, a probable member of the nearby young Horologium association. From previously obtained JHK-band colors and the magnitude…

Astrophysics · Physics 2009-11-10 Ralph Neuhaeuser , Eike Guenther

We have obtained high contrast images of four nearby, faint, and very low mass objects 2MASSJ04351455-1414468, SDSSJ044337.61+000205.1, 2MASSJ06085283-2753583 and 2MASSJ06524851-5741376 (here after 2MASS0435-14, SDSS0443+00, 2MASS0608-27…

This study presents observations of two possible substellar survivors of post-main sequence engulfment, currently orbiting white dwarf stars. Infrared and optical spectroscopy of GD 1400 reveal a 9.98 h orbital period, where the benchmark…

Solar and Stellar Astrophysics · Physics 2022-12-21 N. Walters , J. Farihi , T. R. Marsh , E. Breedt , P. W. Cauley , T. von Hippel , J. J. Hermes

White dwarf main-sequence (WDMS) binaries provide important laboratories for studying binary evolution and the formation of low-mass white dwarfs. In this work, we identify 654 reliable WDMS candidates with FGK-type companions from an…

We present a near-IR spectroscopic analysis of the intriguing DO white dwarf RE J0503-285. The IR spectrum fails to reveal evidence of the presence of a spatially unresolved, cool, late-type companion. Hence we have placed an approximate…

Astrophysics · Physics 2009-11-11 Paul Dobbie , Matt Burleigh , Andrew Levan , Martin Barstow , Ralf Napiwotzki , Ivan Hubeny , . , .

The determination of the brown dwarf binary fraction may contribute to the understanding of the substellar formation mechanisms. Unresolved brown dwarf binaries may be revealed through their peculiar spectra or the discrepancy between…

Solar and Stellar Astrophysics · Physics 2015-11-18 E. Manjavacas , B. Goldman , J. M. Alcalá , M. R. Zapatero-Osorio , V. J. S. Béjar , D. Homeier , M. Bonnefoy , R. L. Smart , T. Henning , F. Allard

The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at finding hot subdwarf stars with massive compact companions like massive white dwarfs (M > 1.0 Msun), neutron stars or stellar mass black…

PG 2131+066 is a composite-spectrum binary with a hot pulsating PG 1159-type pre-white dwarf and an early M-type main sequence star. Analysis of Whole Earth Telescope observations of the pulsating pre-white dwarf component provided an…

Astrophysics · Physics 2009-10-31 M. Reed , Steven D. Kawaler , M. Sean O'Brien

We report on Keck optical BVRI images and spectroscopy of the companion of the binary millisecond pulsar PSR J0218+4232. A faint bluish (V=24.2, B-V=0.25) counterpart is observed at the pulsar location. Spectra of this counterpart reveal…

Astrophysics · Physics 2011-05-23 C. G. Bassa , M. H. van Kerkwijk , S. R. Kulkarni

We present spatially resolved photometric and spectroscopic observations of two wide brown dwarf binaries uncovered by the SIMP near-infrared proper motion survey. The first pair (SIMP J1619275+031350AB) has a separation of 0.691" (15.2 AU)…

We present a photometric analysis of 19 DA and 13 DAO white dwarfs (WDs) with effective temperatures exceeding 60 kK, building on the spectral analysis reported in the first paper of this two-part study. By examining archival light curves…

Solar and Stellar Astrophysics · Physics 2026-01-19 Semih Filiz , Nicole Reindl , David Jones , Paulina Sowicka , Matti Dorsch , Thomas Rauch , Klaus Werner

New near-infrared large-area sky surveys (e.g. UKIDSS, CFBDS, WISE) go deeper than 2MASS and aim at detecting brown dwarfs lurking in the Solar neighbourhood which are even fainter than the latest known T-type objects, so-called Y dwarfs.…

Astrophysics of Galaxies · Physics 2015-05-18 R. -D. Scholz

We report the discovery of a wide (approximately 400 AU projected separation), common proper motion companion to the nearby M dwarf LHS 2803 (PSO J207.0300-13.7422). This object was discovered during our census of the local T dwarf…

SDSS J080531.84+481233.0 is a peculiar L-type dwarf that exhibits unusually blue near-infrared and mid-infrared colors and divergent optical (L4) and near-infrared (L9.5) spectral classifications. These peculiar spectral traits have been…

Astrophysics · Physics 2009-06-23 Adam J. Burgasser

We report the discovery of the wide L1.5+L4.5 binary 2MASS J15200224-4422419AB, identified during spectroscopic followup of high proper motion sources selected from the Two Micron All Sky Survey. This source was independently identified by…

Astrophysics · Physics 2009-01-19 Adam J. Burgasser , Dagny L. Looper , J. Davy Kirkpatrick , Michael C. Liu

This paper presents results of a near-infrared imaging survey for low mass stellar and substellar companions to white dwarfs. A wide field proper motion survey of 261 white dwarfs was capable of directly detecting companions at orbital…

Astrophysics · Physics 2009-11-11 J. Farihi , E. E. Becklin , B. Zuckerman
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