Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit.

Xie F, Di Marco A, La Monaca F, Liu K, Muleri F, Bucciantini N, Romani RW, Costa E, Rankin J, Soffitta P, Bachetti M, Di Lalla N, Fabiani S, Ferrazzoli R, Gunji S, Latronico L, Negro M, Omodei N, Pilia M, Trois A, Watanabe E, Agudo I, Antonelli LA, Baldini L, Baumgartner WH, Bellazzini R, Bianchi S, Bongiorno SD, Bonino R, Brez A, Capitanio F, Castellano S, Cavazzuti E, Ciprini S, De Rosa A, Del Monte E, Di Gesu L, Donnarumma I, Doroshenko V, Dovčiak M, Ehlert SR, Enoto T, Evangelista Y, Garcia JA, Hayashida K, Heyl J, Iwakiri W, Jorstad SG, Karas V, Kitaguchi T, Kolodziejczak JJ, Krawczynski H, Liodakis I, Maldera S, Manfreda A, Marin F, Marinucci A, Marscher AP, Marshall HL, Massaro F, Matt G, Mitsuishi I, Mizuno T, Ng CY, O'Dell SL, Oppedisano C, Papitto A, Pavlov GG, Peirson AL, Perri M, Pesce-Rollins M, Petrucci PO, Possenti A, Poutanen J, Puccetti S, Ramsey BD, Ratheesh A, Sgró C, Slane P, Spandre G, Tamagawa T, Tavecchio F, Taverna R, Tawara Y, Tennant AF, Thomas NE, Tombesi F, Tsygankov SS, Turolla R, Vink J, Weisskopf MC, Wu K, Zane S

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DOI
10.1038/s41586-022-05476-5
Published
2022 Dec
Container
Nature
Publisher
Not recorded
Open access
unknown

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BibTeX

@article{allodium:10.1038/s41586-022-05476-5,
  title = {Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit.},
  author = {Xie F and Di Marco A and La Monaca F and Liu K and Muleri F and Bucciantini N and Romani RW and Costa E and Rankin J and Soffitta P and Bachetti M and Di Lalla N and Fabiani S and Ferrazzoli R and Gunji S and Latronico L and Negro M and Omodei N and Pilia M and Trois A and Watanabe E and Agudo I and Antonelli LA and Baldini L and Baumgartner WH and Bellazzini R and Bianchi S and Bongiorno SD and Bonino R and Brez A and Capitanio F and Castellano S and Cavazzuti E and Ciprini S and De Rosa A and Del Monte E and Di Gesu L and Donnarumma I and Doroshenko V and Dovčiak M and Ehlert SR and Enoto T and Evangelista Y and Garcia JA and Hayashida K and Heyl J and Iwakiri W and Jorstad SG and Karas V and Kitaguchi T and Kolodziejczak JJ and Krawczynski H and Liodakis I and Maldera S and Manfreda A and Marin F and Marinucci A and Marscher AP and Marshall HL and Massaro F and Matt G and Mitsuishi I and Mizuno T and Ng CY and O'Dell SL and Oppedisano C and Papitto A and Pavlov GG and Peirson AL and Perri M and Pesce-Rollins M and Petrucci PO and Possenti A and Poutanen J and Puccetti S and Ramsey BD and Ratheesh A and Sgró C and Slane P and Spandre G and Tamagawa T and Tavecchio F and Taverna R and Tawara Y and Tennant AF and Thomas NE and Tombesi F and Tsygankov SS and Turolla R and Vink J and Weisskopf MC and Wu K and Zane S},
  year = {2022},
  journal = {Nature},
  doi = {10.1038/s41586-022-05476-5},
  url = {https://doi.org/10.1038/s41586-022-05476-5}
}

RIS

TY  - JOUR
TI  - Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit.
AU  - Xie F
AU  - Di Marco A
AU  - La Monaca F
AU  - Liu K
AU  - Muleri F
AU  - Bucciantini N
AU  - Romani RW
AU  - Costa E
AU  - Rankin J
AU  - Soffitta P
AU  - Bachetti M
AU  - Di Lalla N
AU  - Fabiani S
AU  - Ferrazzoli R
AU  - Gunji S
AU  - Latronico L
AU  - Negro M
AU  - Omodei N
AU  - Pilia M
AU  - Trois A
AU  - Watanabe E
AU  - Agudo I
AU  - Antonelli LA
AU  - Baldini L
AU  - Baumgartner WH
AU  - Bellazzini R
AU  - Bianchi S
AU  - Bongiorno SD
AU  - Bonino R
AU  - Brez A
AU  - Capitanio F
AU  - Castellano S
AU  - Cavazzuti E
AU  - Ciprini S
AU  - De Rosa A
AU  - Del Monte E
AU  - Di Gesu L
AU  - Donnarumma I
AU  - Doroshenko V
AU  - Dovčiak M
AU  - Ehlert SR
AU  - Enoto T
AU  - Evangelista Y
AU  - Garcia JA
AU  - Hayashida K
AU  - Heyl J
AU  - Iwakiri W
AU  - Jorstad SG
AU  - Karas V
AU  - Kitaguchi T
AU  - Kolodziejczak JJ
AU  - Krawczynski H
AU  - Liodakis I
AU  - Maldera S
AU  - Manfreda A
AU  - Marin F
AU  - Marinucci A
AU  - Marscher AP
AU  - Marshall HL
AU  - Massaro F
AU  - Matt G
AU  - Mitsuishi I
AU  - Mizuno T
AU  - Ng CY
AU  - O'Dell SL
AU  - Oppedisano C
AU  - Papitto A
AU  - Pavlov GG
AU  - Peirson AL
AU  - Perri M
AU  - Pesce-Rollins M
AU  - Petrucci PO
AU  - Possenti A
AU  - Poutanen J
AU  - Puccetti S
AU  - Ramsey BD
AU  - Ratheesh A
AU  - Sgró C
AU  - Slane P
AU  - Spandre G
AU  - Tamagawa T
AU  - Tavecchio F
AU  - Taverna R
AU  - Tawara Y
AU  - Tennant AF
AU  - Thomas NE
AU  - Tombesi F
AU  - Tsygankov SS
AU  - Turolla R
AU  - Vink J
AU  - Weisskopf MC
AU  - Wu K
AU  - Zane S
PY  - 2022
JO  - Nature
DO  - 10.1038/s41586-022-05476-5
UR  - https://doi.org/10.1038/s41586-022-05476-5
ER  -

APA

F, X., A, D. M., F, L. M., K, L., F, M., N, B., RW, R., E, C., J, R., P, S., M, B., N, D. L., S, F., R, F., S, G., L, L., M, N., N, O., M, P., A, T., E, W., I, A., LA, A., L, B., WH, B., R, B., S, B., SD, B., R, B., A, B., F, C., S, C., E, C., S, C., A, D. R., E, D. M., L, D. G., I, D., V, D., M, D., SR, E., T, E., Y, E., JA, G., K, H., J, H., W, I., SG, J., V, K., T, K., JJ, K., H, K., I, L., S, M., A, M., F, M., A, M., AP, M., HL, M., F, M., G, M., I, M., T, M., CY, N., SL, O., C, O., A, P., GG, P., AL, P., M, P., M, P., PO, P., A, P., J, P., S, P., BD, R., A, R., C, S., P, S., G, S., T, T., F, T., R, T., Y, T., AF, T., NE, T., F, T., SS, T., R, T., J, V., MC, W., K, W., & S, Z. (2022). Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit.. Nature. https://doi.org/10.1038/s41586-022-05476-5

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