Results 91 to 100 of about 98,496 (277)
The Astrophysical Journal Letters, 2023 We present a pulse timing analysis of NICER observations of the accreting millisecond X-ray pulsar SAX J1808.4−3658 during the outburst that started on 2022 August 19.
Giulia Illiano +21 more
doaj +1 more source
A massive millisecond pulsar in an eccentric binary [PDF]
, 2016 The recent discovery of a population of eccentric (e ~ 0.1) millisecond pulsar (MSP) binaries with low-mass white dwarf companions in the Galactic field represents a challenge to evolutionary models that explain MSP formation as recycling: all such ...
E. Barr +7 more
semanticscholar +1 more source
XMM‐Newton Observations of the Peculiar Be X‐Ray Binary A0538‐66
Astronomische Nachrichten, Volume 346, Issue 1, January 2025.ABSTRACT A0538‐66 is a neutron star/Be x‐ray binary located in the Large Magellanic Cloud and, since its discovery in the 70s, it showed a peculiar behavior that makes it a unique object in the high‐mass x‐ray binaries scene: the extremely eccentric orbit (e=0.72$$ e=0.72 $$), the short spin period of the neutron star (P=69$$ P=69 $$ ms), the episodes ...
Michela Rigoselli +3 more
wiley +1 more source
The XinJiang Astronomical Observatory NSRT Pulsar Data Archive
Advances in Astronomy, Volume 2019, Issue 1, 2019., 2019 The sensitivity of our pulsar observation system with typical integration time of 16 minutes has reached 0.4 mJy after we have upgraded the receiver cooling system of NanShan 25‐m radio telescope (NSRT) at Xinjiang Astronomical Observatory (XAO) in 2002. About 280 pulsars were observed after the upgrade.
Hailong Zhang +6 more
wiley +1 more source
Searching for Millisecond Pulsars: Surveys, Techniques and Prospects [PDF]
, 2013 Searches for millisecond pulsars (which we here loosely define as those with periods $
Lorimer, D. R., Lynch, R. S, Stovall, K.
core +3 more sources
A millisecond pulsar in an extremely wide binary system [PDF]
, 2016 We report on 22 yrs of radio timing observations of the millisecond pulsar J1024−0719 by the telescopes participating in the European Pulsar Timing Array (EPTA).
C. Bassa +36 more
semanticscholar +1 more source
The Role of XMM–Newton in the Investigation of Persistent BeXRBs
Astronomische Nachrichten, Volume 346, Issue 1, January 2025.ABSTRACT The persistent BeXRBs are a class of high‐mass X‐ray binaries (HMXRBs), which are characterized by persistent low X‐ray luminosities (LX~1034$$ {L}_{\mathrm{X}}\sim {10}^{34} $$ erg s −1$$ {}^{-1} $$) and wide (Porb>$$ {P}_{\mathrm{orb}}> $$ 30 days), almost circular orbits. In these sources the NS is slowly rotating (with Pspin$$ {P}_{\mathrm{
Nicola La Palombara +4 more
wiley +1 more source
Observations of Radio Magnetars with the Deep Space Network
Advances in Astronomy, Volume 2019, Issue 1, 2019., 2019 The Deep Space Network (DSN) is a worldwide array of radio telescopes which supports NASA’s interplanetary spacecraft missions. When the DSN antennas are not communicating with spacecraft, they provide a valuable resource for performing observations of radio magnetars, searches for new pulsars at the Galactic Center, and additional pulsar‐related ...
Aaron B. Pearlman +3 more
wiley +1 more source
The second millisecond pulsar [PDF]
Nature, 1983 On the principle that no celestial object is unique, the discovery of another millisecond pulsar is overdue. That reported on page 417 has an unexpected interest.
openaire +1 more source
The NANOGrav 15 yr Data Set: Observations and Timing of 68 Millisecond Pulsars
The Astrophysical Journal Letters, 2023 We present observations and timing analyses of 68 millisecond pulsars (MSPs) comprising the 15 yr data set of the North American Nanohertz Observatory for Gravitational Waves (NANOGrav).
Gabriella Agazie +100 more
doaj +1 more source