Magnetic topologies of two weak-line T Tauri stars TAP 4 and TAP 40

Autor: Yue Xiang, Shenghong Gu, J-F Donati, G A J Hussain, A Collier Cameron, the MaT Y S S E collaboration

We present a Zeeman-Doppler imaging study of two weak-line T Tauri stars TAP 4 and TAP 40, based on the high-resolution spectropolarimetric observations with ESPaDOnS at the Canada-France-Hawaii Telescope in November 2013, in the framework of the MaT

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::26a1c88d33a81168857eadd177d4a47f
https://hdl.handle.net/10023/26970

Polarimetry of hydrogen-poor superluminous supernovae

Autor: Pursiainen, M., Leloudas, G., Cikota, A., Bulla, M., Inserra, C., Patat, F., Wheeler, J. C., Aamer, A., Gal-Yam, A., Maund, J., Nicholl, M., Schulze, S., Sollerman, J., Yang, Y.

Publikováno v: Pursiainen, M, Leloudas, G, Cikota, A, Bulla, M, Inserra, C, Patat, F, Wheeler, J C, Aamer, A, Gal-Yam, A, Maund, J, Nicholl, M, Schulze, S, Sollerman, J & Yang, Y 2023, ' Polarimetry of hydrogen-poor superluminous supernovae ', Astronomy and Astrophysics, vol. 674, A81 . https://doi.org/10.1051/0004-6361/202345945

We present linear polarimetry for seven hydrogen-poor superluminous supernovae (SLSNe-I). For SN 2017gci, for which we present two epochs of spectropolarimetry at +3 d and +29 d post-peak in rest frame, accompanied by four epochs of imaging polarimet

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a013667ef088bb798b7500aa712387c5
https://orbit.dtu.dk/en/publications/408e5bc4-a35f-4514-94c2-d61a5152bbde

Polarized emission from strongly magnetized sources

Autor: Roberto Taverna, Roberto Turolla, Silvia Zane, Valery Suleimanov, Alexander Y. Potekhin

Publikováno v: Proceedings of the International Astronomical Union. 16:276-279

Anomalous X-ray pulsars (AXPs) and Soft gamma repeaters (SGRs) form together a single class of astrophysical sources, commonly associated to magnetars. New-generation X-ray polarimeters will play a key role in assessing the nature of these sources by

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::735e114f8016a92f0ae3d669978e532b
https://doi.org/10.1017/s174392132200028x

The Calern Asteroid Polarisation Survey : state of the art: An updated catalogue of asteroid polarimetric data

Autor: Bendjoya, Ph., Cellino, A., Rivet, Jean-Pierre, Devogèle, M., Bagnulo, S., Abe, L., Vernet, D., Gil-Hutton, R., Veneziani, A.

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 665, pp.A66. ⟨10.1051/0004-6361/202142960⟩

International audience; Context. The Calern Asteroid Polarimetric Survey (CAPS), a collaboration between the INAF Astrophysical Observatory of Torino (Italy) and the Observatoire de la Côte d’Azur (Nice, France), has produced new asteroid polarime

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______2191::e78f7f37f19c5a835aea1b1a2ed67aab
https://hal.science/hal-03832764/file/2022_BCRBetAl22a_CAPS_AandA_V06_Resubmitted.pdf

Polarimetry of the superluminous transient ASASSN-15lh

Autor: D. Malesani, Ferdinando Patat, Jesper Sollerman, A. de Ugarte Postigo, Justyn R. Maund, Giorgos Leloudas

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
instname
Maund, J R, Leloudas, G, Malesani, D B, Patat, F, Sollerman, J & Postigo, A D U 2020, ' Polarimetry of the superluminous transient ASASSN-15lh ', Monthly Notices of the Royal Astronomical Society, vol. 498, no. 3, pp. 3730–3735 . https://doi.org/10.1093/mnras/staa2517

ASASSN-15lh is the intrinsically brightest transient observed to date. Despite being the subject of concerted photometric and spectroscopic observing campaigns, there is still significant debate about the true nature of this transient and the mechani

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cdc3be3f3ec23e2771a834143209c018
https://doi.org/10.1093/mnras/staa2517