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We report the discovery of the likely white dwarf companions to radio millisecond pulsars 47 Tuc Q and 47 Tuc S in the globular cluster 47 Tucanae. These blue stars were found in near-ultraviolet images from the Hubble Space Telescope for…

We search for stellar and substellar companions of young nearby stars to investigate stellar multiplicity and formation of stellar and substellar companions. We detect common proper-motion companions of stars via multi-epoch imaging. Their…

Astrophysics · Physics 2009-11-13 T. Eisenbeiss , A. Seifahrt , M. Mugrauer , T. O. B. Schmidt , R. Neuhaeuser , T. Roell

The Fermi $\gamma$-ray source 1FGL J1417.7--4407 (J1417) is a compact X-ray binary with a neutron star primary and a red giant companion in a $\sim$5.4 day orbit. This initial conclusion, based on optical and X-ray data, was confirmed when…

We report the discovery of an eclipsing binary -- PTF1 J072456$+$125301-- composed of a subdwarf B (sdB) star ($g'=17.2^m$) with a faint companion. Subdwarf B stars are core helium-burning stars, which can be found on the extreme horizontal…

Solar and Stellar Astrophysics · Physics 2015-08-19 M. Schindewolf , D. Levitan , U. Heber , H. Drechsel , V. Schaffenroth , T. Kuper , T. Prince

We present the first multi-band optical light curves of PSR J1622-0315, among the most compact known redback binary millisecond pulsars, with an orbital period Porb=3.9 h. We find a flux modulation with two maxima per orbital cycle and a…

High Energy Astrophysical Phenomena · Physics 2023-09-06 Marco Turchetta , Manuel Linares , Karri Koljonen , Bidisha Sen

We present Keck spectroscopic measurements of the millisecond pulsar binary J2215+5135. These data indicate a neutron-star (NS) mass M_NS=1.6Mo, much less than previously estimated. The pulsar heats the companion face to T_D~9000K; the…

High Energy Astrophysical Phenomena · Physics 2015-08-19 Roger W. Romani , Melissa L. Graham , Alexei V. Filippenko , Matthew Kerr

We present spectra of the white-dwarf companions of the radio pulsars 0655+64 and 0820+02. For the latter, we find a spectrum showing strong lines of hydrogen, i.e., that of a DA star. From modelling these lines, the mass of a white dwarf…

Astrophysics · Physics 2009-10-28 M. H. van Kerkwijk , S. R. Kulkarni

We present spectroscopic and photometric observations of the optical counterpart to PSR J1911-5958A, a millisecond pulsar located towards the globular cluster NGC 6752. We measure radial velocities from the spectra and determine the…

Astrophysics · Physics 2009-11-11 C. G. Bassa , M. H. van Kerkwijk , D. Koester , F. Verbunt

Using an Extreme Ultraviolet Explorer (EUVE) spectrum, we confirm the identification of a white dwarf companion to the B9.5V star 16 Dra (HD150100), and constrain its surface temperature to lie between 29,000K and 35,000K. This is the third…

Astrophysics · Physics 2007-05-23 Matt Burleigh , Martin Barstow

We report the discovery of a new black-widow millisecond pulsar, PSR J1544-2555, associated with the Fermi-LAT source 4FGL J1544.2-2554. Optical, radio, and gamma-ray observations confirmed its nature as a compact spider binary system.…

We obtained spectra of ASASSN-V J205543.90+240033.5 (J2055), a system that shows photometric variations similar to the white dwarf (WD) pulsar AR Scorpii (Kato et al. arXiv:2109.03979). Our spectra display a continuum rising steeply toward…

Solar and Stellar Astrophysics · Physics 2021-10-18 R. Mark Wagner , Peter Garnavich , John R. Thorstensen , Colin Littlefield , Paula Szkody

We study the evolution of close binary systems in order to account for the existence of the recently observed binary system containing the most massive millisecond pulsar ever detected, PSR J0740+6620, and its ultra-cool helium white dwarf…

Solar and Stellar Astrophysics · Physics 2020-06-03 M. Echeveste , M. L. Novarino , O. G. Benvenuto , M. A. De Vito

We report on deep VLT observations of the fields of two nearby, isolated millisecond pulsars PSR J1744-1134 and PSR J1024-0719. Both objects are old neutron stars with characteristic age $\tau \ge 10^9$ yr and have relatively high spin-down…

Astrophysics · Physics 2011-05-23 F. K. Sutaria , A. Ray , A. Reisenegger , G. Hertling , H. Quintana , D. Minniti

We present ULTRACAM multiband optical photometry of two transitional millisecond pulsars, PSR J1023+0038 and PSR J1227$-$4853, taken while both were in their radio pulsar states. The light curves show significant asymmetry about the flux…

We present new 0.9-2.45 $\mu$m spectroscopy ($R \sim 1000$), and $Y$, $J$, $H$, $K_s$, $L^\prime$ photometry, obtained at Gemini North, of three low-mass brown dwarf companions on wide orbits around young stars of the Upper Scorpius OB…

Several redback and black widow millisecond pulsar binaries have episodes of flaring in X-rays and optical. We initially detected such behavior from the Fermi selected redback candidate 1FGL J0523.5$-$2529 during optical time-series…

High Energy Astrophysical Phenomena · Physics 2022-08-31 Jules P. Halpern , Karen I. Perez , Slavko Bogdanov

PSR J1928+1815 is a 10.55 ms millisecond pulsar in a 3.6 hr orbit with a massive ($1.0$-$1.6\,M_{\odot}$) companion that produces extended radio eclipses. The companion, proposed to be a stripped helium star, is undetected in optical and…

Solar and Stellar Astrophysics · Physics 2026-04-07 Pranav Nagarajan , Kareem El-Badry , Jim Fuller , Yunlang Guo , Thomas M. Tauris

We report the discovery of PSR J1909-3744, a 2.95 millisecond pulsar in a nearly circular 1.53 day orbit. Its narrow pulse width of 43 microseconds allows pulse arrival times to be determined with great accuracy. We have spectroscopically…

Astrophysics · Physics 2009-11-10 B. A. Jacoby , M. Bailes , M. H. van Kerkwijk , S. Ord , A. Hotan , S. R. Kulkarni , S. B. Anderson

We present timing and orbital phase-resolved polarimetry of the millisecond pulsar (MSP) J2101$-$4802, having a spin period of 9.48~ms and dispersion measure (DM) $25.05\ \mathrm{pc\ cm^{-3}}$ discovered with the Giant Meter Radio Telescope…

We have discovered a new X-ray emitting compact binary that is the likely counterpart to the unassociated Fermi-LAT GeV $\gamma$-ray source 4FGL J1120.0-2204, the second brightest Fermi source that still remains formally unidentified. Using…

High Energy Astrophysical Phenomena · Physics 2022-03-02 Samuel J. Swihart , Jay Strader , Elias Aydi , Laura Chomiuk , Kristen C. Dage , Adam Kawash , Kirill V. Sokolovsky , Elizabeth C. Ferrara
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