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Related papers: Spitzer Planet Limits around the Pulsating White D…

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We present preliminary limits on the presence of planets around white dwarf stars using the IRAC photometer on the Spitzer space telescope. Planets emit strongly in the mid-infrared which allows their presence to be detected as an excess at…

Astrophysics · Physics 2007-05-23 F. Mullally , Ted von Hippel , D. E. Winget

We present limits on planetary companions to pulsating white dwarf stars. A subset of these stars exhibit extreme stability in the period and phase of some of their pulsation modes; a planet can be detected around such a star by searching…

The potential existence of a giant planet orbiting within a few AU of a stellar remnant has profound implications for both the survival and possible regeneration of planets during post-main sequence stellar evolution. This paper reports…

Earth and Planetary Astrophysics · Physics 2012-06-15 J. Farihi , J. P. Subasavage , E. P. Nelan , H. C. Harris , C. C. Dahn , J. Nordhaus , D. S. Spiegel

We examine 14 hot white dwarfs for signs of infrared excess using the Spitzer Space Telescope. Twelve of the objects are massive white dwarfs which have been suggested to be the result of binary mergers. The remaining two objects are…

Astrophysics · Physics 2008-11-26 Brad M. S. Hansen , Shri Kulkarni , Sloane Wiktorowicz

The formation scenarios for single low-mass (M < 0.45 Msol) white dwarfs include enhanced mass loss from a metal-rich progenitor star or a common envelope phase of a solar-like star with a close-in massive planet or a brown dwarf. Both…

Solar and Stellar Astrophysics · Physics 2014-11-20 Mukremin Kilic , Warren R. Brown , B. McLeod

We present mid-infrared photometry of 124 white dwarf stars with Spitzer Space Telescope. Objects were observed simultaneously at 4.5 and 8.0um with sensitivities better than 1 mJy. This data can be used to test models of white dwarf…

We present optical high-speed photometry of three millisecond pulsars with low-mass ($< 0.3 M_{\odot}$) white dwarf companions, bringing the total number of such systems with follow-up time-series photometry to five. We confirm the…

This paper presents a sensitive and comprehensive IRAC 3-8 $\mu$m photometric survey of white dwarfs for companions in the planetary mass regime with temperatures cooler than the known T dwarfs. The search focuses on descendents of…

Astrophysics · Physics 2009-11-13 J. Farihi , E. E. Becklin , B. Zuckerman

For the last three years we have performed a survey for young (<3 Gyrs) giant planets around nearby white dwarfs with HST, Spitzer, and VLT. Direct HST/NICMOS imaging of the seven white dwarfs in the Hyades gave no evidence for companions…

Astrophysics · Physics 2007-05-23 S. Friedrich , H. Zinnecker , S. Correia , W. Brandner , M. Burleigh , M. McCaughrean

We report on a search for pulsars at the positions of eight low-mass white dwarfs and one higher-mass white dwarf with the 100-m Effelsberg Radio Telescope. These systems have orbital parameters suggesting that their unseen companions are…

Pulsars in close, eccentric binary systems are usually assumed to have another neutron star as a companion. These double neutron star binaries have proven to be the best laboratories for experimental General Relativity and are the most…

Astrophysics · Physics 2009-10-31 M. H. van Kerkwijk , S. R. Kulkarni

We present Spitzer IRAC photometry of white dwarf remnants of 14 stars with M = 3-5 Msol. We do not detect mid-infrared excess around any of our targets. By demanding a 3 sigma photometric excess at 4.5 micron for unresolved companions, we…

Solar and Stellar Astrophysics · Physics 2014-11-20 Mukremin Kilic , Andrew Gould , Detlev Koester

We report Spitzer Space Telescope photometry of eleven externally-polluted white dwarfs. Of the nine stars for which we have IRAC photometry, we find that GD 40, GD 133 and PG 1015+161 each has an infrared excess that can be understood as…

Astrophysics · Physics 2009-06-23 M. Jura , J. Farihi , B. Zuckerman

The pulsar B1620-26 has two companions, one of stellar mass and one of planetary mass. We detected the stellar companion using Hubble Space Telescope observations. The color and magnitude of the stellar companion indicate that it is an…

We report identification of the optical counterpart to the companion of the millisecond pulsar J2317+1439. At the timing position of the pulsar, we find an object with $g=22.96\pm0.05$, $r=22.86\pm0.04$ and $i=22.82\pm0.05$. The magnitudes…

Solar and Stellar Astrophysics · Physics 2017-06-28 S. Dai , M. C. Smith , S. Wang , S. Okamoto , R. X. Xu , Y. L. Yue , J. F. Liu

Fluxes and upper limits in the wavelength range from 3.6 to 70 microns from the Spitzer Space Telescope are provided for twenty solar-mass Pleiades members. One of these stars shows a probable mid-IR excess and two others have possible…

Spitzer Space Observatory IRAC and MIPS photometric observations are presented for 20 white dwarfs with T < 20,000 K and metal-contaminated photospheres. A warm circumstellar disk is detected at GD 16 and likely at PG 1457-086, while the…

Earth and Planetary Astrophysics · Physics 2011-02-11 J. Farihi , M. Jura , B. Zuckerman

Infrared excesses around white dwarf stars indicate the presence of various astrophysical objects of interest, including companions and debris disks. In this second paper of a series, we present follow-up observations of infrared excess…

We report limits in the planetary-mass regime for companions around the nearest single white dwarf to the Sun, van Maanen's star (vMa 2), from deep J-band imaging with Gemini North and Spitzer IRAC mid-IR photometry. We find no resolved…

We present the discovery of a white dwarf companion at 3.6" from GJ3346, a nearby ($\pi\sim$42 mas) K star observed with SPHERE@VLT as part of an open time survey for faint companions to objects with significant proper motion discrepancies…

Solar and Stellar Astrophysics · Physics 2020-03-04 M. Bonavita , C. Fontanive , S. Desidera , V. D'Orazi , A. Zurlo , K. Muzic , B. Biller , R. Gratton , D. Mesa , A. Sozzetti
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