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Related papers: A new extremely low-mass white dwarf in the NLTT c…

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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

The nature of the excess near-infrared emission associated with the magnetic white dwarf commonly known as SDSS 1212 is investigated primarily through spectroscopy, and also via photometry. The inferred low mass secondary in this system has…

Astrophysics · Physics 2009-11-13 J. Farihi , M. R. Burleigh , D. W. Hoard

We present a grid of evolutionary tracks for low-mass white dwarfs with helium cores in the mass range from 0.179 to 0.414 M_sun. The lower mass limit is well suited for comparison with white dwarf companions of millisecond pulsars (MSP).…

Astrophysics · Physics 2007-05-23 T. Driebe , T. Bloecker , D. Schoenberner

We present the results of a search for cool white dwarfs in the United Kingdom InfraRed Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS) Large Area Survey (LAS). The UKIDSS LAS photometry was paired with the Sloan Digital Sky Survey…

Solar and Stellar Astrophysics · Physics 2015-05-27 S. K. Leggett , N. Lodieu , P. -E. Tremblay , P. Bergeron , A. Nitta

We present full evolutionary calculations appropriate for the study of hot hydrogen-deficent DO white dwarfs, PG 1159 stars, and DB white dwarfs. White dwarf sequences are computed for a wide range of stellar masses and helium envelopes on…

Solar and Stellar Astrophysics · Physics 2014-11-20 L. G. Althaus , J. A. Panei , M. M. Miller Bertolami , E. García-Berro , A. H. Córsico , A. D. Romero , S. O. Kepler , R. D. Rohrmann

We present a model atmosphere analysis of cool hydrogen-rich white dwarfs observed at the Very Large Telescope (VLT) with the X-shooter spectrograph. The intermediate-dispersion and high signal-to-noise ratio of the spectra allowed us to…

Solar and Stellar Astrophysics · Physics 2015-06-03 Adela Kawka , Stephane Vennes

We report the spectroscopic confirmation of four further white dwarf members of Praesepe. This brings the total number of confirmed white dwarf members to eleven making this the second largest collection of these objects in an open cluster…

We present the orbit and properties of 2MASS J050051.85-093054.9, establishing it as the closest (d ~ 71 pc) extremely low mass white dwarf to the Sun. We find that this star is hydrogen-rich with Teff ~ 10 500 K, log g ~ 5.9, and,…

Solar and Stellar Astrophysics · Physics 2020-05-06 Adela Kawka , Jeffrey D. Simpson , Stephane Vennes , Michael S. Bessell , Gary S. Da Costa , Anna F. Marino , Simon J. Murphy

With the Keck I Low-Resolution Imaging Spectrometer we have observed nine white dwarf candidates in the very rich open cluster NGC 2099 (M37). The spectroscopy shows seven to be DA white dwarfs, one to be a DB white dwarf, and one to be a…

Solar and Stellar Astrophysics · Physics 2016-03-23 Jeffrey D. Cummings , Jason S. Kalirai , P. -E. Tremblay , Enrico Ramirez-Ruiz , P. Bergeron

Using the SDSS and Pan-STARRS1 survey data, we found a likely companion of the recently discovered binary $\gamma$-ray radio-loud millisecond pulsar J0621+2514. Its visual brightness is about 22 mag. The broad band magnitudes and colours…

Solar and Stellar Astrophysics · Physics 2018-07-05 A. V. Karpova , D. A. Zyuzin , Yu. A. Shibanov , A. Yu. Kirichenko , S. V. Zharikov

The recycled pulsar PSR J2222-0137 is one of the closest known neutron stars, with a parallax distance of $267_{-0.9}^{+1.2}\,$pc and an edge-on orbit. We measure the Shapiro delay in the system through pulsar timing with the Green Bank…

We present a detailed analysis of 108 helium-line (DB) white dwarfs based on model atmosphere fits to high signal-to-noise optical spectroscopy. We derive a mean mass of 0.67 Mo for our sample, with a dispersion of only 0.09 Mo. White…

Two of the possibilities for the formation of low-mass ($M_{\star}\lesssim 0.5\,M_{\odot}$) hydrogen-deficient white dwarfs are the occurrence of a very-late thermal pulse after the asymptotic giant-branch phase or a late helium-flash onset…

Solar and Stellar Astrophysics · Physics 2020-07-01 Tiara Battich , Leandro G. Althaus , Alejandro H. Córsico

We present the discovery of a new double detonation progenitor system consisting of a hot subdwarf B (sdB) binary with a white dwarf companion with an P=76.34179(2) min orbital period. Spectroscopic observations are consistent with an sdB…

We present the results of a photometric and spectroscopic study of the white dwarf candidate members of the intermediate age open clusters NGC3532 and NGC2287. Of the nine objects investigated, it is determined that six are probable members…

Solar and Stellar Astrophysics · Physics 2009-11-13 P. D. Dobbie , R. Napiwotzki , M. R. Burleigh , K. Williams , R. G. Sharp , M. A. Barstow , S. L. Casewell , I. Hubeny

We report the discovery of an ultra-cool white dwarf in the COMBO-17 survey. So far, only seven objects have been discovered in this rare category of white dwarfs, which are characterized by strong flux depression in the far-red and…

Astrophysics · Physics 2009-11-11 C. Wolf

We present the discovery and spectroscopic identification of two very high proper motion ancient white dwarf stars, found in a systematic proper motion survey. Their kinematics and apparent magnitude clearly indicate that they are halo…

Astrophysics · Physics 2009-10-31 Rodrigo Ibata , Michael Irwin , Olivier Bienayme , Ralf Scholz , Jean Guibert

We present 2MASS J11151597+1937266, a recently identified low-surface gravity L dwarf, classified as an L2$\gamma$ based on Sloan Digital Sky Survey optical spectroscopy. We confirm this spectral type with near-infrared spectroscopy, which…

Fifty-two magnetic white dwarfs have been identified in spectroscopic observations from the Sloan Digital Sky Survey (SDSS) obtained between mid-2002 and the end of 2004, including Data Releases 2 and 3. Though not as numerous nor as…

We report the discovery of a subtle infrared excess associated with the young white dwarf EC\,05365--4749 at 3.35 and 4.6\,$\mu$m. Follow-up spectroscopic observations are consistent with a hydrogen atmosphere white dwarf of effective…

Solar and Stellar Astrophysics · Physics 2016-11-08 E. Dennihy , John H. Debes , B. H. Dunlap , P. Dufour , Johanna K. Teske , J. C. Clemens
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