Astrofísica

A NICER View on the 2020 Magnetar-like Outburst of PSR J1846-0258

Enviado por Valeria.salas en Jue, 12/28/2023 - 16:18

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Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector

Enviado por Valeria.salas en Jue, 12/07/2023 - 10:24

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Main features of magnetospheric dynamics in the conditions of pressure balance

Enviado por Valeria.salas en Jue, 12/07/2023 - 10:15

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The first mm detection of a neutron star high-mass X-ray binary

Enviado por roberto.bernal en Mié, 10/25/2023 - 11:22

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Magnetic reconnection plasmoid model for Sagittarius A* flares

Enviado por roberto.bernal en Mié, 10/25/2023 - 11:20

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Spectroscopic analysis of VVV CL001 cluster with MUSE

Enviado por roberto.bernal en Mar, 08/01/2023 - 08:12

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Spirals and Clumps in V960 Mon: Signs of Planet Formation via Gravitational Instability around an FU Ori Star?

Enviado por roberto.bernal en Mar, 08/01/2023 - 08:09

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Resolving the binary components of the outbursting protostar HBC 494 with ALMA

Enviado por roberto.bernal en Mar, 08/01/2023 - 08:08

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The ALMA view of MP Mus (PDS 66): A protoplanetary disk with no visible gaps down to 4 au scales

Enviado por roberto.bernal en Mar, 08/01/2023 - 08:07

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Inner edges of planetesimal belts: collisionally eroded or truncated?

Enviado por roberto.bernal en Mar, 08/01/2023 - 08:05

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Astrofísica

A NICER View on the 2020 Magnetar-like Outburst of PSR J1846-0258

Ionospheric response modeling under eclipse conditions: Evaluation of 14 December 2020, total solar eclipse prediction over the South American sector

Main features of magnetospheric dynamics in the conditions of pressure balance

The first mm detection of a neutron star high-mass X-ray binary

Magnetic reconnection plasmoid model for Sagittarius A* flares

Spectroscopic analysis of VVV CL001 cluster with MUSE

Spirals and Clumps in V960 Mon: Signs of Planet Formation via Gravitational Instability around an FU Ori Star?

Resolving the binary components of the outbursting protostar HBC 494 with ALMA

The ALMA view of MP Mus (PDS 66): A protoplanetary disk with no visible gaps down to 4 au scales

Inner edges of planetesimal belts: collisionally eroded or truncated?

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