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Vela X-1 in depth: a review article on an outstanding object

Authors: Martínez-Núñez, Silvia; Kretschmar, Peter; El Mellah, I.; Fuerst, F.; Grinberg, V.; Sander, A.; van den Eijnden, J.; +5 Authors

Vela X-1 in depth: a review article on an outstanding object

Abstract

In this poster, we will summarise the review paper entitled: "Revisiting the archetypical wind accretor Vela X-1 in depth. Case study of a well-known X-ray binary and the limits of our knowledge." The paper, published in late 2021 in Astronomy and Astrophysics journal, triggered a discussion amongst the editors of Astronomy and Astrophysics leading to the creation of a new type of review article on uniquely interesting objects. In the paper we have: provided a thoughtful compilation of the knowledge of the Vela X-1 system and its modelling published over decades; added new information derived from public data or catalogues, including an updated distance and spectral classification based on the Gaia EDR3 release; and identified specific avenues of future research that could help to clarify open questions.

SMN acknowledges funding by the Spanish Ministry MCIU under project RTI2018-096686-B-C21 (MCIU/AEI/FEDER, UE), co-funded by FEDER funds and by the Unidad de Excelencia María de Maeztu, ref. MDM-2017-0765.

Country
France
Keywords

accretion disks, X-rays: individuals: Vela X-1, outflows, X-rays: individuals: Vela X-1; X-rays: binaries; stars: winds; outflows; accretion; accretion disks; Astrophysics - High Energy Astrophysical Phenomena; Astrophysics - Solar and Stellar Astrophysics, [PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph], X-rays: binaries, Astrophysics - Solar and Stellar Astrophysics, accretion, stars: winds, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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