Zobrazeno 1 - 10
of 40
pro vyhledávání: '"M. Pakull"'
Autor:
A. Nebot Gómez-Morán, C. Motch, X. Barcons, F. J. Carrera, M. T. Ceballos, M. Cropper, N. Grosso, P. Guillout, O. Hérent, S. Mateos, L. Michel, J. P. Osborne, M. Pakull, F.-X. Pineau, J. P. Pye, T. P. Roberts, S. R. Rosen, A. D. Schwope, M. G. Watson, N. Webb
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics, 2013, 553, A12
Astronomy & astrophysics, 2013, Vol.553, pp.A12 [Peer Reviewed Journal]
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
instname
Astronomy and Astrophysics, 2013, 553, A12
Astronomy & astrophysics, 2013, Vol.553, pp.A12 [Peer Reviewed Journal]
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
Many different classes of X-ray sources contribute to the Galactic landscape at high energies. Although the nature of the most luminous X-ray emitters is now fairly well understood, the population of low-to-medium X-ray luminosity (LX = 1027-34 erg s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::97de6502ebcfc484cfc4fa2673b36961
http://hdl.handle.net/10261/109200
http://hdl.handle.net/10261/109200
Autor:
M. Pakull, R. Pallavicini
Publikováno v:
Cool Stars, Stellar Systems, and the Sun ISBN: 9783540129073
A new instrument capable of providing high spectral resolution observations of relatively bright objects became operational in 1982 at the European Southern Observatory (ESO) at La Silla (Chile). This is the Coud~ Echelle Spectrometer (CES), which in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e56c2afd59b6260af948c21ba8af439f
https://doi.org/10.1007/3-540-12907-3_186
https://doi.org/10.1007/3-540-12907-3_186
Autor:
I. A. Smith, S. D. Ryder, S. J. Tingay, M. Böttcher, E. P. Liang, M. Pakull, A. Stacy, Charles Meegan, Chryssa Kouveliotou, Neil Gehrels
We discuss our radio (Australia Telescope Compact Array and Australian Long Baseline Array) and X-ray (XMM-Newton) monitoring observations of the unusual ultraluminous supernova SN 1978K in NGC 1313 at ~25 years after the explosion. SN 1978K is a rar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96471f08dcd5136ee3140637809cf82d
Autor:
M. G. Watson, J.-L. Auguères, J. Ballet, X. Barcons, D. Barret, M. Boer, Th. Boller, G. E. Bromage, H. Brunner, F. J. Carrera, M. S. Cropper, M. Denby, M. Ehle, M. Elvis, A. C. Fabian, M. J. Freyberg, P. Guillout, J.-M. Hameury, G. Hasinger, D. A. Hinshaw, T. Maccacaro, K. O. Mason, R. G. McMahon, L. Michel, L. Mirioni, J. P. Mittaz, C. Motch, J.-F. Olive, J. P. Osborne, C. G. Page, M. Pakull, B. H. Perry, M. Pierre, W. Pietsch, J. P. Pye, A. M. Read, T. P. Roberts, S. R. Rosen, J.-L. Sauvageot, A. D. Schwope, K. Sekiguchi, G. C. Stewart, I. Stewart, I. Valtchanov, M. J. Ward, R. S. Warwick, R. G. West, N. E. White, D. M. Worrall
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2001, 365 (1), pp.L51-L59. ⟨10.1051/0004-6361:20000067⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2001, 365 (1), pp.L51-L59. ⟨10.1051/0004-6361:20000067⟩
This paper describes the performance of XMM-Newton for serendipitous surveys and summarises the scope and potential of the XMM-Newton Serendipitous Survey. The role of the Survey Science Centre (SSC) in the XMM-Newton project is outlined. The SSC's f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c7cdf2d84f9ef8d4138ca6b426ff996
https://hal.archives-ouvertes.fr/hal-03118651
https://hal.archives-ouvertes.fr/hal-03118651
Publikováno v:
Symposium - International Astronomical Union. 155:496-496
We report on the discovery of a new PG 1159 star in the ROSAT XRT all sky survey and give results of a model atmosphere analysis. The X-ray source RX J2117.1+3412 is relatively faint (0.33 cnts−1) and extremely soft. Ground based optical follow-up
Publikováno v:
Monthly Notices of the Royal Astronomical Society
On presente les resultats d'observations photometriques de l'associe optique de la source RX transitoire recurrente A0538-66. Trois sursauts ont ete observes en avril et mai 1982, aucun entre octobre 1982 et juin 1983. On note une diminution seculair
Publikováno v:
Advances in Space Research. 8:405-409
The X-ray source LMC X-2 was observed with EXOSAT for -8hours on February 2nd, 1984 with simultaneous photometric and spectroscopic optical coverage. The source was seen at a luminosity of L x ∼ 1.5 10 38 erg.s −1 with a mean X-ray spectrum which
Publikováno v:
Space Science Reviews. 40:229-232
Publikováno v:
Space Science Reviews. 40:239-243
Publikováno v:
X-Ray Astronomy in the Exosat Era ISBN: 9789401089067
We present preliminary results from V-band CCD photometric observations of several low-mass X-ray binaries with faint optical counterparts obtained at ESO and CFHT from February to September 1984. LMCX-2 exhibits large (0.3–0.5 magnitude) variation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f998fbdf2a5e6458cf145f2888031d43
https://doi.org/10.1007/978-94-009-5448-9_32
https://doi.org/10.1007/978-94-009-5448-9_32