X-ray pulsar

[High Energy Astrophysical Phenomena Papers @PRXI]

Exploring the magnetic field of the ultraluminous X-ray pulsar NGC 4631 X-8

Amar Deo Chandra
https://t.co/QoJRxiUmNX [𝚊𝚜𝚝𝚛𝚘-𝚙𝚑.𝙷𝙴]

[Phys.org @physorg_com]

#A newly detected pulsating ultraluminous #X-ray source, X-8, in galaxy NGC 4631 exhibits rapid spin-up and extreme luminosity, offering insights into super-Eddington accretion physics. @arxiv https://t.co/Ci7xHOeFyQ https://t.co/a6kFFv7Puk

[Trentymus Kostorus @TrentKostorus]

A recent study on the ultraluminous X-ray pulsar (ULXP) RX J0209.6-7427 estimated its surface magnetic field strength to be between 2.4 and 4 × 10^13 Gauss.

➡️: https://t.co/HVcaqAjxy4

[X-ray pulsar @RayPulsar]

The discovery of pulsars is one of the most exciting astronomical discoveries of the 20th century!

[X-ray pulsar @RayPulsar]

Jocelyn Bell Burnell discovered pulsars (manifesting as periodic “scruff” on the chart records) nearly six decades ago (28th Nov 1967) as a graduate student in radio astronomy at Cambridge.
https://t.co/MypuFbfCl4

[High Energy Astrophysical Phenomena Papers @PRXI]

On the origin of super-global spin-up trends of X-ray pulsars in HMXB systems. https://t.co/uUaNFivkKA

[High Energy Astrophysical Phenomena Papers @PRXI]

Formation of twin compact stars in low-mass X-ray binaries: Implications on eccentric and isolated millisecond pulsar populations. https://t.co/Sqx1wZawBy

[High Energy Astrophysical Phenomena Papers @PRXI]

The full jet production cycle observed during fast state transitions in the black hole X-ray binary MAXI J1348$-$630. https://t.co/4Yw1f2lhGJ

[NASA Universe @NASAUniverse]

#OTD in 1967, Jocelyn Bell Burnell discovered pulsars, the rapidly spinning cores of dead stars that emit pulses of light with ultraprecise timing. Decades later, we’re still learning about what matter is like under such extreme conditions: https://t.co/DvG9lWTzGP

[BBC Oxfordshire @BBCOxford]

Oxford Professor Dame Jocelyn Bell-Burnell discovered the first pulsar in 1967 - a discovery so important in our understanding of the universe that it would earn a Nobel Prize.
Watch her story here: https://t.co/zhU0nGi444

[High Energy Astrophysical Phenomena Papers @PRXI]

Long-term spin-down and low luminosity regime in the Be/X-ray binary pulsar GX 304-1. https://t.co/8vXVtPCKmQ

[High Energy Astrophysical Phenomena Papers @PRXI]

A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614--3329. https://t.co/pIXwnv4ZjE

[arXiv astro-ph @_arXiv_astro_ph]

[2301.10678] Amar Deo Chandra, Jayashree Roy, P. C. Agrawal: AstroSat observations of the Be/X-ray binary XTE J1946+274 during 2018 and 2021 outbursts https://t.co/pmbwNaN4V4 https://t.co/6LaTdWW586 #astro_ph_HE

[X-ray pulsar @RayPulsar]

Jocelyn Bell Burnell discovered pulsars (manifesting as periodic “scruff” on the chart records) in 1967 as a graduate student in radio astronomy at Cambridge. Discovery of pulsars is one of the most exciting astronomical discoveries of the 20th century!

[Physics In History @PhysInHistory]

Today, in 1967, the first pulsating radio source (pulsar) was detected by an alert graduate student, Jocelyn Bell, then working under the direction of Prof. Anthony Hewish at the Mullard Radio Astronomy Observatory, Cambridge, England.

[arXiver @arXiver]

The unaltered pulsar: GRO J1750-27, a super-critical X-ray neutron star that does not blink an eye [HEAP] https://t.co/crUeeI4cnb

[arXiv astro-ph @_arXiv_astro_ph]

[2211.09491] Birendra Chhotaray, Gaurava K. Jaisawal, Neeraj Kumari et al.: Optical and X-ray studies of Be/X-ray binary 1A 0535+262 during its 2020 giant outburst https://t.co/9cOUIKvW7D https://t.co/OjPBfYcRYE #astro_ph_HE

[arXiver @arXiver]

Monte-Carlo simulations on possible collimation effects of outflows to fan-beamed emission of... [HEAP] https://t.co/4eLY5VrMTO

[arXiver @arXiver]

Bright X-ray Pulsars: how outflows influence beaming, pulsations and pulse phase lags [HEAP] https://t.co/aqbD1d3yRw

[arXiver @arXiver]

Spectral properties of the Be/X-ray pulsar 2S 1553-542 during Type II outbursts [HEAP] https://t.co/h6aCsnkxtf

[Nature Astronomy @NatureAstronomy]

Initial results from IXPE (NASA/ASI mission) leverage the power of X-ray polarimetry to constrain the accretion geometry in X-ray pulsar Her X-1. The results also indicate a misalignment of the spin, magnetic & orbital axes. @doroshv3, Poutanen et al.: https://t.co/o3PjXyvp2B