Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Lerothodi L. Leeuw"'
Publikováno v:
Proceedings of the International Astronomical Union. 15:379-382
Presented here, is a summary of discussions at African Astronomical Society (AfAS) Science Business Meeting, Addis Ababa, Ethiopia, 10-11 October 2019. This summary was deliberated with delegates of the International Astronomical Union (IAU) Symposiu
Autor:
Lerothodi L. Leeuw
Publikováno v:
Multilingual Universities in South Africa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e665b6fbe9c879326af462e1f17de81a
https://doi.org/10.21832/9781783091669-012
https://doi.org/10.21832/9781783091669-012
Autor:
Henry E. Matthews, Roger H. Hildebrand, Lerothodi L. Leeuw, Jacqueline A. Davidson, C. Darren Dowell
Publikováno v:
ISLAND UNIVERSES ISBN: 9781402055720
SHARC II, 350-micron continuum and archival HST J-H band maps are presented of NGC 3656, the brightest of our sample of six elliptical galaxies for which resolved CO gas disks have recently been detected with 7''-spatial-resolution, interferometry ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9cd8736bda93c0deb1bf688602800e72
https://doi.org/10.1007/978-1-4020-5573-7_67
https://doi.org/10.1007/978-1-4020-5573-7_67
Autor:
Lerothodi L. Leeuw
Publikováno v:
Mass-Losing Pulsating Stars and their Circumstellar Matter ISBN: 9789401039680
Near- to mid-infrared photometric properties are preliminarily exhibited of IRAS Miras that lie within -7.°3 < b < +1° and 282.°5 < l < 285.°5. Tentative O-/C-rich classifications based on K — L versus [12 μm] — [25 μm] colours and pulsatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::07f793713e4dbac44c8d9f188d095ab8
https://doi.org/10.1007/978-94-010-0139-7_46
https://doi.org/10.1007/978-94-010-0139-7_46
Autor:
Lerothodi L. Leeuw
Publikováno v:
Proceedings of the International Astronomical Union. 10:126-126
We present GALEX ultraviolet (UV) emission results of star-formation in a small sample of nearby, gas-rich early-type galaxies. The first observational evidence of star-formation in this sample was presented by Leeuw et al.2008, using 350 μm continu