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相关论文: PG 1258+593 and its common proper motion magnetic …

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SDSSJ125733.63+542850.5 (hereafter SDSSJ1257+5428) is a compact white dwarf binary from the Sloan Digital Sky Survey that exhibits high-amplitude radial velocity variations on a period of 4.56 hours. While an initial analysis suggested the…

太阳与恒星天体物理 · 物理学 2015-05-18 T. R. Marsh , B. T. Gaensicke , D. Steeghs , J. Southworth , D. Koester , V. Harris , L. Merry

SDSS 1257+5428 is a white dwarf in a close orbit with a companion that has been suggested to be a neutron star. If so, it hosts the closest known neutron star, and its existence implies a great abundance of similar systems and a rate of…

星系天体物理 · 物理学 2015-05-18 S. R. Kulkarni , M. H. van Kerkwijk

We identify SDSSJ121010.1+334722.9 as an eclipsing post-common-envelope binary, with an orbital period of P ~ 3 hrs, containing a very cool, low-mass, DAZ white dwarf and a low-mass main-sequence star of spectral type M5. A model atmosphere…

We present the confirmation of SDSS J222551.65+001637.7AB as a closely separated, resolved, white dwarf-brown dwarf binary. We have obtained spectroscopy from GNIRS and seeing-limited $K_s$-band imaging from NIRI on Gemini North. The target…

太阳与恒星天体物理 · 物理学 2023-01-18 Jenni R. French , Sarah L. Casewell , Trent J. Dupuy , John H. Debes , Elena Manjavacas , Emily C. Martin , Siyi Xu

Abridged: We report the discovery of two, new, rare, wide, double-degenerate binaries that each contain a magnetic and a non-magnetic star. The components of SDSSJ092646.88+132134.5 + J092647.00+132138.4 and SDSSJ150746.48+521002.1 +…

The magnetic white dwarf SDSS J121209.31+013627.7 exhibits a weak, narrow Halpha emission line whose radial velocity and strength are modulated on a period of ~90 minutes. Though indicative of irradiation on a nearby companion, no cool…

天体物理学 · 物理学 2009-11-13 G. D. Schmidt , P. Szkody , N. M. Silvestri , M. C. Cushing , J. Liebert , P. S. Smith

In a search for common proper motion companions using the VISTA Hemisphere Survey and 2MASS catalogs we have identified a very red (J-Ks=2.47 mag) late-L dwarf companion of a previously unrecognized M dwarf VHS J125601.92-125723.9, located…

We demonstrate that the previously identified L/T transition brown dwarf SDSS J213154.43-011939.3 (SDSS 2131-0119) is a widely separated (82.3'', $\sim$3830 au) common proper motion companion to the low-mass star NLTT 51469, which we reveal…

太阳与恒星天体物理 · 物理学 2019-05-22 B. Gauza , V. J. S. Béjar , A. Pérez-Garrido , N. Lodieu , R. Rebolo , M. R. Zapatero Osorio , B. Pantoja , S. Velasco , J. S. Jenkins

We report the discovery of a wide pair (93 arcsec angular separation) of extremely cool ($T_{eff}<4000$ K) white dwarfs with a very large common proper motion ($\sim1.9$ arcsec/yr). The objects were discovered in a high proper motion survey…

天体物理学 · 物理学 2009-11-07 R. -D. Scholz , G. P. Szokoly , M. Andersen , R. Ibata , M. Irwin

The Hubble Space Telescope observation of the double white dwarf (WD) binary SDSS J125733.63$+$542850.5 reveal that the massive WD has a surface gravity log$g_1\sim8.7$ (which implies a mass of $M_1\sim1.06~{\rm M_\odot}$) and an effective…

高能天体物理现象 · 物理学 2018-05-16 Long Jiang , Wen-Cong Chen , Xiang-Dong Li

We report on nine wide common proper motion systems containing late-type M, L, or T companions. We confirm six previously reported companions, and identify three new systems. The ages of these systems are determined using diagnostics for…

We report the discovery of five white dwarf + ultracool dwarf systems identified as common proper motion wide binaries in the Gaia Catalogue of Nearby Stars. The discoveries include a white dwarf + L subdwarf binary, VVV 1256-62AB, a…

Studies of cool white dwarfs in the solar neighbourhood have placed a limit on the age of the Galactic disk of 8-9 billion years. However, determining their cooling ages requires the knowledge of their effective temperatures, masses, radii,…

The system WDS 16329+0315 is an old, nearby quintuple physical system in the thick Galactic disc formed by a close-resolved, triple primary of solar metallicity, namely HD 149162, and a very wide, common proper motion, secondary pair,…

太阳与恒星天体物理 · 物理学 2018-08-20 R. González-Peinado , J. A. Caballero , D. Montes , C. Cifuentes

We report on photometric and spectroscopic observations of white dwarf companions to four binary radio millisecond pulsars, leading to the discovery of companions to PSRs J0614-3329, J1231-1411 and J2017+0603. We place limits on the…

高能天体物理现象 · 物理学 2015-12-09 C. G. Bassa , J. Antoniadis , F. Camilo , I. Cognard , D. Koester , M. Kramer , S. R. Ransom , B. W. Stappers

We report the identification of SDSS J121929.45+471522.8 as the third apparently isolated magnetic (B~18.5+/-1.0,MG) white dwarf exhibiting Zeeman-split Balmer emission lines. The star shows coherent variability at optical wavelengths with…

We present the discovery of the first T dwarf + white dwarf binary system LSPM 1459+0857AB, confirmed through common proper motion and spectroscopy. The white dwarf is a high proper motion object from the LSPM catalogue that we confirm…

We report the discovery of the ninth pre-polar, consisting of a late-type ZAMS secondary and a magnetic white dwarf. The white dwarf accretes at extreme low rate, dot{M} ~ 10**-14 Msun/yr, from the wind of the companion donor star. The…

太阳与恒星天体物理 · 物理学 2011-03-28 A. D. Schwope , A. Nebot Gomez-Moran , M. R. Schreiber , B. T. Gaensicke

We report on the discovery of the companion star to the millisecond pulsar PSR J1835-3259B in the Galactic globular cluster NGC 6652. Taking advantage of deep photometric archival observations acquired through the Hubble Space Telescope in…

高能天体物理现象 · 物理学 2023-05-17 J. Chen , M. Cadelano , C. Pallanca , F. Ferraro , B. Lanzoni , A. Istrate , M. Burgay , P. Freire , T. Gautam , A. Possenti , A. Ridolfi

We have used multi-epoch images from the Infrared Array Camera on board the Spitzer Space Telescope to search for substellar companions to stars in the solar neighborhood based on common proper motions. Through this work, we have discovered…

星系天体物理 · 物理学 2015-05-27 K. L. Luhman , A. J. Burgasser , J. J. Bochanski
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