onr:"swepub:oai:DiVA.org:kth-28605"
Sökning: onr:"swepub:oai:DiVA.org:kth-28605" > Detection of the Sm...
- 1 av 1
- Föregående post
- Nästa post
- Till träfflistan
| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 09058naa a2202305 4500 | |
| 001 | oai:DiVA.org:kth-28605 | |
| 003 | SwePub | |
| 008 | 110117s2010 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-286052 URI |
| 024 | 7 | a https://doi.org/10.1051/0004-6361/2010148552 DOI |
| 040 | a (SwePub)kth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Abdo, A. A.4 aut |
| 245 | 1 0 | a Detection of the Small Magellanic Cloud in gamma-rays with Fermi/LAT |
| 264 | c 2010-11-16 | |
| 264 | 1 | b EDP Sciences,c 2010 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20110117 | |
| 520 | a Context. The flux of gamma rays with energies greater than 100 MeV is dominated by diffuse emission coming from cosmic-rays (CRs) illuminating the interstellar medium (ISM) of our Galaxy through the processes of Bremsstrahlung, pion production and decay, and inverse-Compton scattering. The study of this diffuse emission provides insight into the origin and transport of cosmic rays. Aims. We searched for gamma-ray emission from the Small Magellanic Cloud (SMC) in order to derive constraints on the cosmic-ray population and transport in an external system with properties different from the Milky Way. Methods. We analysed the first 17 months of continuous all-sky observations by the Large Area Telescope (LAT) of the Fermi mission to determine the spatial distribution, flux and spectrum of the gamma-ray emission from the SMC. We also used past radio synchrotron observations of the SMC to study the population of CR electrons specifically. Results. We obtained the first detection of the SMC in high-energy gamma rays, with an integrated >100 MeV flux of (3.7 +/- 0.7) x 10(-8) ph cm(-2) s(-1), with additional systematic uncertainty of <= 16%. The emission is steady and from an extended source similar to 3 degrees in size. It is not clearly correlated with the distribution of massive stars or neutral gas, nor with known pulsars or supernova remnants, but a certain correlation with supergiant shells is observed. Conclusions. The observed flux implies an upper limit on the average CR nuclei density in the SMC of similar to 15% of the value measured locally in the Milky Way. The population of high-energy pulsars of the SMC may account for a substantial fraction of the gamma-ray flux, which would make the inferred CR nuclei density even lower. The average density of CR electrons derived from radio synchrotron observations is consistent with the same reduction factor but the uncertainties are large. From our current knowledge of the SMC, such a low CR density does not seem to be due to a lower rate of CR injection and rather indicates a smaller CR confinement volume characteristic size. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a acceleration of particles | |
| 653 | a cosmic rays | |
| 653 | a Magellanic Clouds | |
| 653 | a gamma rays: general | |
| 653 | a Astronomy and astrophysics | |
| 653 | a Astronomi och astrofysik | |
| 700 | 1 | a Ackermann, M.4 aut |
| 700 | 1 | a Ajello, M.4 aut |
| 700 | 1 | a Baldini, L.4 aut |
| 700 | 1 | a Ballet, J.4 aut |
| 700 | 1 | a Barbiellini, G.4 aut |
| 700 | 1 | a Bastieri, D.4 aut |
| 700 | 1 | a Bechtol, K.4 aut |
| 700 | 1 | a Bellazzini, R.4 aut |
| 700 | 1 | a Berenji, B.4 aut |
| 700 | 1 | a Blandford, D.4 aut |
| 700 | 1 | a Bloom, E. D.4 aut |
| 700 | 1 | a Bonamente, E.4 aut |
| 700 | 1 | a Borgland, A. W.4 aut |
| 700 | 1 | a Bouvier, A.4 aut |
| 700 | 1 | a Brandt, T. J.4 aut |
| 700 | 1 | a Bregeon, J.4 aut |
| 700 | 1 | a Brez, A.4 aut |
| 700 | 1 | a Brigida, M.4 aut |
| 700 | 1 | a Bruel, P.4 aut |
| 700 | 1 | a Buehler, R.4 aut |
| 700 | 1 | a Buson, S.4 aut |
| 700 | 1 | a Caliandro, G. A.4 aut |
| 700 | 1 | a Cameron, R. A.4 aut |
| 700 | 1 | a Caraveo, P. A.4 aut |
| 700 | 1 | a Carrigan, S.4 aut |
| 700 | 1 | a Casandjian, J. M.4 aut |
| 700 | 1 | a Cecchi, C.4 aut |
| 700 | 1 | a Celik, Oe.4 aut |
| 700 | 1 | a Charles, E.4 aut |
| 700 | 1 | a Chekhtman, A.4 aut |
| 700 | 1 | a Cheung, C. C.4 aut |
| 700 | 1 | a Chiang, J.4 aut |
| 700 | 1 | a Ciprini, S.4 aut |
| 700 | 1 | a Claus, R.4 aut |
| 700 | 1 | a Cohen-Tanugi, J.4 aut |
| 700 | 1 | a Conrad, J.4 aut |
| 700 | 1 | a Dermer, C. D.4 aut |
| 700 | 1 | a de Palma, F.4 aut |
| 700 | 1 | a Digel, S. W.4 aut |
| 700 | 1 | a do Couto e Silva, E.4 aut |
| 700 | 1 | a Drell, P. S.4 aut |
| 700 | 1 | a Dubois, R.4 aut |
| 700 | 1 | a Dumora, D.4 aut |
| 700 | 1 | a Favuzzi, C.4 aut |
| 700 | 1 | a Fegan, S. J.4 aut |
| 700 | 1 | a Fukazawa, Y.4 aut |
| 700 | 1 | a Funk, S.4 aut |
| 700 | 1 | a Fusco, P.4 aut |
| 700 | 1 | a Gargano, F.4 aut |
| 700 | 1 | a Gasparrini, D.4 aut |
| 700 | 1 | a Gehrels, N.4 aut |
| 700 | 1 | a Germani, S.4 aut |
| 700 | 1 | a Giglietto, N.4 aut |
| 700 | 1 | a Giordano, F.4 aut |
| 700 | 1 | a Giroletti, M.4 aut |
| 700 | 1 | a Glanzman, T.4 aut |
| 700 | 1 | a Godfrey, G.4 aut |
| 700 | 1 | a Grenier, I. A.4 aut |
| 700 | 1 | a Grondin, M. -H4 aut |
| 700 | 1 | a Grove, J. E.4 aut |
| 700 | 1 | a Guiriec, S.4 aut |
| 700 | 1 | a Hadasch, D.4 aut |
| 700 | 1 | a Harding, A. K.4 aut |
| 700 | 1 | a Hayashida, M.4 aut |
| 700 | 1 | a Hays, E.4 aut |
| 700 | 1 | a Horan, D.4 aut |
| 700 | 1 | a Hughes, R. E.4 aut |
| 700 | 1 | a Jean, P.4 aut |
| 700 | 1 | a Johannesson, G.4 aut |
| 700 | 1 | a Johnson, A. S.4 aut |
| 700 | 1 | a Johnson, W. N.4 aut |
| 700 | 1 | a Kamae, T.4 aut |
| 700 | 1 | a Katagiri, H.4 aut |
| 700 | 1 | a Kataoka, J.4 aut |
| 700 | 1 | a Kerr, M.4 aut |
| 700 | 1 | a Knoedlseder, J.4 aut |
| 700 | 1 | a Kuss, M.4 aut |
| 700 | 1 | a Lande, J.4 aut |
| 700 | 1 | a Latronico, L.4 aut |
| 700 | 1 | a Lee, S. -H4 aut |
| 700 | 1 | a Lemoine-Goumard, M.4 aut |
| 700 | 1 | a Garde, M. Llena4 aut |
| 700 | 1 | a Longo, F.4 aut |
| 700 | 1 | a Loparco, F.4 aut |
| 700 | 1 | a Lovellette, M. N.4 aut |
| 700 | 1 | a Lubrano, P.4 aut |
| 700 | 1 | a Makeev, A.4 aut |
| 700 | 1 | a Martin, P.4 aut |
| 700 | 1 | a Mazziotta, M. N.4 aut |
| 700 | 1 | a McEnery, J. E.4 aut |
| 700 | 1 | a Michelson, P. F.4 aut |
| 700 | 1 | a Mitthumsiri, W.4 aut |
| 700 | 1 | a Mizuno, T.4 aut |
| 700 | 1 | a Monte, C.4 aut |
| 700 | 1 | a Monzani, M. E.4 aut |
| 700 | 1 | a Morselli, A.4 aut |
| 700 | 1 | a Moskalenko, I. V.4 aut |
| 700 | 1 | a Murgia, S.4 aut |
| 700 | 1 | a Nakamori, T.4 aut |
| 700 | 1 | a Naumann-Godo, M.4 aut |
| 700 | 1 | a Nolan, P. L.4 aut |
| 700 | 1 | a Norris, J. P.4 aut |
| 700 | 1 | a Nuss, E.4 aut |
| 700 | 1 | a Ohsugi, T.4 aut |
| 700 | 1 | a Okumura, A.4 aut |
| 700 | 1 | a Omodei, N.4 aut |
| 700 | 1 | a Orlando, E.4 aut |
| 700 | 1 | a Ormes, J. F.4 aut |
| 700 | 1 | a Panetta, J. H.4 aut |
| 700 | 1 | a Parent, D.4 aut |
| 700 | 1 | a Pelassa, V.4 aut |
| 700 | 1 | a Pepe, M.4 aut |
| 700 | 1 | a Pesce-Rollins, M.4 aut |
| 700 | 1 | a Piron, F.4 aut |
| 700 | 1 | a Porter, T. A.4 aut |
| 700 | 1 | a Raino, S.4 aut |
| 700 | 1 | a Rando, R.4 aut |
| 700 | 1 | a Razzano, M.4 aut |
| 700 | 1 | a Reimer, A.4 aut |
| 700 | 1 | a Reimer, O.4 aut |
| 700 | 1 | a Reposeur, T.4 aut |
| 700 | 1 | a Ripken, J.4 aut |
| 700 | 1 | a Ritz, S.4 aut |
| 700 | 1 | a Romani, R. W.4 aut |
| 700 | 1 | a Sadrozinski, H. F. -W4 aut |
| 700 | 1 | a Sander, A.4 aut |
| 700 | 1 | a Parkinson, P. M. Saz4 aut |
| 700 | 1 | a Scargle, J. D.4 aut |
| 700 | 1 | a Sgro, C.4 aut |
| 700 | 1 | a Siskind, E. J.4 aut |
| 700 | 1 | a Smith, D. A.4 aut |
| 700 | 1 | a Smith, P. D.4 aut |
| 700 | 1 | a Spandre, G.4 aut |
| 700 | 1 | a Spinelli, P.4 aut |
| 700 | 1 | a Strickman, M. S.4 aut |
| 700 | 1 | a Strong, A. W.4 aut |
| 700 | 1 | a Suson, D. J.4 aut |
| 700 | 1 | a Takahashi, H.4 aut |
| 700 | 1 | a Takahashi, T.4 aut |
| 700 | 1 | a Tanaka, T.4 aut |
| 700 | 1 | a Thayer, J. B.4 aut |
| 700 | 1 | a Thayer, J. G.4 aut |
| 700 | 1 | a Thompson, D. J.4 aut |
| 700 | 1 | a Tibaldo, L.4 aut |
| 700 | 1 | a Torres, D. F.4 aut |
| 700 | 1 | a Tosti, G.4 aut |
| 700 | 1 | a Tramacere, A.4 aut |
| 700 | 1 | a Uchiyama, Y.4 aut |
| 700 | 1 | a Usher, T. L.4 aut |
| 700 | 1 | a Vandenbroucke, J.4 aut |
| 700 | 1 | a Vasileiou, V.4 aut |
| 700 | 1 | a Vilchez, N.4 aut |
| 700 | 1 | a Vitale, V.4 aut |
| 700 | 1 | a Waite, A. P.4 aut |
| 700 | 1 | a Wang, P.4 aut |
| 700 | 1 | a Winer, B. L.4 aut |
| 700 | 1 | a Wood, K. S.4 aut |
| 700 | 1 | a Yang, Z.4 aut |
| 700 | 1 | a Ylinen, Tomiu KTH,Fysik4 aut0 (Swepub:kth)u1vmovqg |
| 700 | 1 | a Ziegler, M.4 aut |
| 710 | 2 | a KTHb Fysik4 org |
| 773 | 0 | t Astronomy and Astrophysicsd : EDP Sciencesg 523, s. A46-q 523<A46-x 0004-6361x 1432-0746 |
| 856 | 4 | u https://www.aanda.org/articles/aa/pdf/2010/15/aa14855-10.pdf |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-28605 |
| 856 | 4 8 | u https://doi.org/10.1051/0004-6361/201014855 |
Hitta via bibliotek
- Astronomy and Astrophysics (Sök värdpublikationen i LIBRIS)
Till lärosätets databas
- 1 av 1
- Föregående post
- Nästa post
- Till träfflistan
Hitta mer i SwePub
- Av författaren/redakt...
- Abdo, A. A.
- Ackermann, M.
- Ajello, M.
- Baldini, L.
- Ballet, J.
- Barbiellini, G.
- visa fler...
- Bastieri, D.
- Bechtol, K.
- Bellazzini, R.
- Berenji, B.
- Blandford, D.
- Bloom, E. D.
- Bonamente, E.
- Borgland, A. W.
- Bouvier, A.
- Brandt, T. J.
- Bregeon, J.
- Brez, A.
- Brigida, M.
- Bruel, P.
- Buehler, R.
- Buson, S.
- Caliandro, G. A.
- Cameron, R. A.
- Caraveo, P. A.
- Carrigan, S.
- Casandjian, J. M ...
- Cecchi, C.
- Celik, Oe.
- Charles, E.
- Chekhtman, A.
- Cheung, C. C.
- Chiang, J.
- Ciprini, S.
- Claus, R.
- Cohen-Tanugi, J.
- Conrad, J.
- Dermer, C. D.
- de Palma, F.
- Digel, S. W.
- do Couto e Silva ...
- Drell, P. S.
- Dubois, R.
- Dumora, D.
- Favuzzi, C.
- Fegan, S. J.
- Fukazawa, Y.
- Funk, S.
- Fusco, P.
- Gargano, F.
- Gasparrini, D.
- Gehrels, N.
- Germani, S.
- Giglietto, N.
- Giordano, F.
- Giroletti, M.
- Glanzman, T.
- Godfrey, G.
- Grenier, I. A.
- Grondin, M. -H
- Grove, J. E.
- Guiriec, S.
- Hadasch, D.
- Harding, A. K.
- Hayashida, M.
- Hays, E.
- Horan, D.
- Hughes, R. E.
- Jean, P.
- Johannesson, G.
- Johnson, A. S.
- Johnson, W. N.
- Kamae, T.
- Katagiri, H.
- Kataoka, J.
- Kerr, M.
- Knoedlseder, J.
- Kuss, M.
- Lande, J.
- Latronico, L.
- Lee, S. -H
- Lemoine-Goumard, ...
- Garde, M. Llena
- Longo, F.
- Loparco, F.
- Lovellette, M. N ...
- Lubrano, P.
- Makeev, A.
- Martin, P.
- Mazziotta, M. N.
- McEnery, J. E.
- Michelson, P. F.
- Mitthumsiri, W.
- Mizuno, T.
- Monte, C.
- Monzani, M. E.
- Morselli, A.
- Moskalenko, I. V ...
- Murgia, S.
- Nakamori, T.
- Naumann-Godo, M.
- Nolan, P. L.
- Norris, J. P.
- Nuss, E.
- Ohsugi, T.
- Okumura, A.
- Omodei, N.
- Orlando, E.
- Ormes, J. F.
- Panetta, J. H.
- Parent, D.
- Pelassa, V.
- Pepe, M.
- Pesce-Rollins, M ...
- Piron, F.
- Porter, T. A.
- Raino, S.
- Rando, R.
- Razzano, M.
- Reimer, A.
- Reimer, O.
- Reposeur, T.
- Ripken, J.
- Ritz, S.
- Romani, R. W.
- Sadrozinski, H. ...
- Sander, A.
- Parkinson, P. M. ...
- Scargle, J. D.
- Sgro, C.
- Siskind, E. J.
- Smith, D. A.
- Smith, P. D.
- Spandre, G.
- Spinelli, P.
- Strickman, M. S.
- Strong, A. W.
- Suson, D. J.
- Takahashi, H.
- Takahashi, T.
- Tanaka, T.
- Thayer, J. B.
- Thayer, J. G.
- Thompson, D. J.
- Tibaldo, L.
- Torres, D. F.
- Tosti, G.
- Tramacere, A.
- Uchiyama, Y.
- Usher, T. L.
- Vandenbroucke, J ...
- Vasileiou, V.
- Vilchez, N.
- Vitale, V.
- Waite, A. P.
- Wang, P.
- Winer, B. L.
- Wood, K. S.
- Yang, Z.
- Ylinen, Tomi
- Ziegler, M.
- visa färre...
- Om ämnet
-
- NATURVETENSKAP
- NATURVETENSKAP
- och Fysik
- och Astronomi astrof ...
- Artiklar i publikationen
- Astronomy and As ...
- Av lärosätet
- Kungliga Tekniska Högskolan
Sök utanför SwePub
- Sök vidare i:
- Google Book Search
- Google Scholar
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
- Copyright © LIBRIS - Nationella bibliotekssystem
- LIBRIS.kb.se
