Zobrazeno 1 - 10
of 184
pro vyhledávání: '"E. Bajaja"'
Conference
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Astronomy & Astrophysics. 414:453-461
The central region and main body of the very symmetrical galaxy NGC 1566 were observed and studied spectropho- tometrically and kinematically. We found that: a) the total masses derived from the Satoh model fitted to the rotation curve, and from the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::10e2b7737119e239e837839aa559f39f
https://doi.org/10.1051/0004-6361:20031644
https://doi.org/10.1051/0004-6361:20031644
Publikováno v:
Astronomy and Astrophysics Supplement Series. 136:179-187
The galaxy NGC 2442 was observed with a REOSC spectrograph, installed in the 2.15 m CASLEO telescope, in order to derive galactic parameters from the observed optical lines and to compare them with the re- sults of radioastronomical observations made
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f6e03c21799d29b9bec76197baeb67ea
https://doi.org/10.1051/aas:1999459
https://doi.org/10.1051/aas:1999459
Autor:
E. Bajaja, R. F. Haynes, Ulrich Klein, Richard Wielebinski, U. R. Buczilowski, R. Wark, D. Malin, L. Sciacca, J. D. Murray, A. J. Hunt, S. R. Wayte, J. I. Harnett
Publikováno v:
Symposium - International Astronomical Union. 140:205-209
We present preliminary results from a number of deep radio polarization surveys being made of the Magellanic Clouds at 2.3 GHz, 4.75 GHz and 8.55 GHz. Extended and linearly polarized radio emission has been found at 2.3 and 4.75 GHz from both the Lar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::61aafc18301123072a90e3c8f3c3552c
https://doi.org/10.1017/s0074180900189983
https://doi.org/10.1017/s0074180900189983
Publikováno v:
Publications of the Astronomical Society of Australia. 9:258-260
We have mapped the southern galaxies NGC 613, 1313, 1433, 1566, 1672 and 2442 in the12CO(J = 1 → 0) transition with the 15-m Swedish European Submillimetre Telescope (SEST). The sample is based on galaxies previously observed in radio continuum wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5738d7d20d04c7f4ef5765d3a8a8bf90
https://doi.org/10.1017/s132335800002405x
https://doi.org/10.1017/s132335800002405x
Autor:
R. Wielebinski, E. Bajaja
Publikováno v:
Symposium - International Astronomical Union. 148:53-55
The structure of the Large Magellanic Cloud (LMC) has posed many questions and has led to many controversial discussions. Although classified as an 'irregular', repeated claims have been made suggesting that the LMC has spiral structure. Furthermore,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ac63923174dceca26ca9cf2de1f9497c
https://doi.org/10.1017/s0074180900200004
https://doi.org/10.1017/s0074180900200004
Autor:
U. Klein, R. F. Haynes, R. Wielebinski, S. R. Wayte, J. I. Harnett, E. Bajaja, J. D. Murray, A. J. Hunt, R. Wark, L. Sciacca, U. R. Buczilowski
Publikováno v:
The Magellanic Clouds ISBN: 9780792311119
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4d8091f3a555ce15a013f66a2c242abe
https://doi.org/10.1007/978-94-011-3432-3_5
https://doi.org/10.1007/978-94-011-3432-3_5
Autor:
R. F. Haynes, S. Wayte, J. I. Harnett, U. Klein, R. Wielebinski, U. R. Buczilowski, E. Bajaja, D. Malin, J. D. Murray, A. J. Hunt, R. Wark, L. Sciacca
Publikováno v:
Galactic and Intergalactic Magnetic Fields ISBN: 9780792307051
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::54c3684e77ccaade4dd5e2e534b684b8
https://doi.org/10.1007/978-94-009-0569-6_62
https://doi.org/10.1007/978-94-009-0569-6_62
Publikováno v:
Symposium - International Astronomical Union. 140:203-204
A region with strong radio polarization in the SW of M31 was observed in the 12CO(1–0) line. The results are compared with the radio continuum, HI and Ha. The CO emission appears to be correlated with the total radio emission, but anticorrelated wi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::54ac5c35cd0d62a1acc87047d8afc45f
https://doi.org/10.1017/s0074180900189971
https://doi.org/10.1017/s0074180900189971
Publikováno v:
Symposium - International Astronomical Union. 31:181-183
The rotation curve observed with the Argentine radio telescope is systematically higher than that found at Parkes. The discrepancy appears to be caused by the difference in frequency resolution of the two receivers.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ef84d80d682f81abcb9b966dd7f110a2
https://doi.org/10.1017/s0074180900100919
https://doi.org/10.1017/s0074180900100919