Zobrazeno 1 - 10
of 86
pro vyhledávání: '"R. Sancisi"'
Autor:
R. Sancisi
Publikováno v:
Symposium - International Astronomical Union. 186:71-80
HI observations are an excellent tool for investigating tidal interactions. Ongoing major and minor interactions which can lead to traumatic mergers or to accretion and the triggering of star formation, show distinct HI signatures. Interactions and m
Publikováno v:
Astronomy & astrophysics supplement series, 126(3), 537-546
We present results of an HI survey of the cluster of galaxies Abell 262, using the Westerbork Synthesis Radio Telescope (WSRT). Eleven galaxies were detected in five fields. In a few cases the gas in these galaxies shows an asymmetrical distribution;
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::21aaf0126f9242c4a542fc8df76d816e
https://research.rug.nl/en/publications/983d3822-386d-4fa9-9838-6a034c067f58
https://research.rug.nl/en/publications/983d3822-386d-4fa9-9838-6a034c067f58
Publikováno v:
New Light on Galaxy Evolution ISBN: 9780792339762
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9cf7bbbbfd68ba0aac40dfe3915cb7e8
https://doi.org/10.1007/978-94-009-0229-9_161
https://doi.org/10.1007/978-94-009-0229-9_161
Autor:
R. Sancisi
Publikováno v:
Morphological and Physical Classification of Galaxies ISBN: 9789401051132
In the last two decades a large number of spiral galaxies have been studied in the 21-cm line. These studies have revealed the density distribution and kinematics of HI and have provided the measurements of the total mass and the mass distribution in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b08e228304e6a03df10e4ffa176e589a
https://doi.org/10.1007/978-94-011-2522-2_19
https://doi.org/10.1007/978-94-011-2522-2_19
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 199:425-433
Autor:
R. Sancisi
Publikováno v:
Symposium - International Astronomical Union. 60:115-128
Expanding shells of neutral hydrogen have been found connected with the associations Per OB2 and Sco OB2. The shells also contain dust and molecules. A model of the spatial configuration and the kinematics of gas, dust and stars is discussed. The sta
Publikováno v:
Symposium - International Astronomical Union. 58:425-430
Maps with 0′.5 resolution are presented of the distribution of neutral hydrogen in two galaxies. The barred spiral NGC 5383 contains much hydrogen, in strong differential rotation, in its outer parts; some H I concentrations with possibly anomalous