Andrei Igoshev

Royal Society University Research Fellow at Newcastle University. I study magnetic fields of neutron stars.

[Andrei Igoshev @ignotur]

@Nekrolm Вы когда договор с юристом подписываете, там написано на какую сумму все застраховано от ошибок.

А наличие посредников не позволяет развернуться бабушкиному скаму. Условная бабушка мошенница будет судится со своими юристами, а не с покупателем.

[Andrei Igoshev @ignotur]

Astro full house: you get articles under consideration in each of three main journals: ApJ, A&A and MNRAS at the same time.

[Andrei Igoshev @ignotur]

Petition: Do not introduce Digital ID cards https://t.co/DxqSXOi29J

[Andrei Igoshev @ignotur]

I am looking for a postdoc in my research group to work on magnetic field evolution in neutron stars. The deadline is 18th March. https://t.co/ml3I9vAc4n

[Andrei Igoshev @ignotur]

Supernova 'rains' could give rise to mysteriously magnetic dead stars https://t.co/Yj96J4AQw6

https://t.co/ubvnCgDnXl

[Nature Astronomy @NatureAstronomy]

Stellar material falling back following SN explosions plays a key role in forming the magnetic fields of some magnetars. X-ray bursts result from their complex fields, produced by a Tayler-Spruit dynamo. @ignotur et al.: https://t.co/8anPKSFPkX @UniofNewcastle @UniversityLeeds

[Andrei Igoshev @ignotur]

Our new configuration describes observational properties of low-field magnetars because we it explains periods, structure of the field, thermal properties as well as it identifies places where the crust yields producing outburst of X-ray emission.

[Andrei Igoshev @ignotur]

Magnetars have the strongest magnetic field in the Universe. But how are these fields formed? We try to answer exactly this question in our recent paper published in @NatureAstronomy
https://t.co/ubvnCgDnXl

[Andrei Igoshev @ignotur]

The footprints of these arcs could be promising places for persistent X-ray emission due to magnetospheric currents.

[Vanessa Graber @drvgraber]

🌟🌟 Are you or anyone you know interested in doing interdisciplinary neutron star research? I am looking to hire 2 postdocs to join me at RHUL in October 2025. One post will focus on cosmic superfluidity, the other on radio pulsar timing. Deadline 28 February 2025. See below.

[Andrei Igoshev @ignotur]

PhD Studentship in Computational Astrophysics – Magnetic Fields and Superconductivity in Neutron Star Cores.

The deadline is 31 January.

If you want to know more details, please directly contact me.

[Andrei Igoshev @ignotur]

Are you interested in doing a PhD on neutron stars and their magnetic fields? Do you know anybody who is? I am looking for a PhD student to start in October 2025 at Newcastle University.

Studentship code is MSP103: https://t.co/GzivTEzi0E

[Vanessa Graber @drvgraber]

🌟🌟 If you or anyone else you know is interested in doing a PhD in neutron star astrophysics and working with me, I am currently looking for 2 PhD students to join me at Royal Holloway for the 2025/2026 academic year. Application deadline is 31 January 2025. More info below.

[Floor Broekgaarden 💫 @FloorAstro]

Applying for PhDs/grad school, postdocs, internships, faculty jobs in Astronomy this fall? Here's a website that aims to list a lot of incredible resources that the astro community has made:
Check out: https://t.co/EnRzSFuL80 [1/4]

[Andrei Igoshev @ignotur]

@mmosc_m @joonas_nattila They are very similar at the mathematical equation level as well. The book “introduction to magnetohydrodynamics” by Davidson has a whole chapter about it.

[Andrei Igoshev @ignotur]

@MHDwizard Yes, we are working on magnetars with Rainer

[Andrei Igoshev @ignotur]

Nature is so ironic. I’m rereading the old paper about magnetar theory where Thompson & Duncan (1995) contrast and compare two first soft gamma repeaters SGR 1806-20 and SGR 0526-66. At that time it was no precise measurements for spin period of 1806-20 so they discuss how this

[Andrei Igoshev @ignotur]

Only three of them were detected until now.

[Andrei Igoshev @ignotur]

Magnetar could have reduced dipole field. In particular, they say “that only 0526-66 has been observed to emit a burst as energetic as the March 5 event”.

The irony is that ten years later 1806-20 emitted a giant flare. These flares are extremely rare.