Zobrazeno 1 - 10
of 26
pro vyhledávání: '"L. Dedes"'
Autor:
L. Dedes, P.M.W. Kalberla
Publikováno v:
EAS Publications Series. 56:209-212
21-cm studies of the Galactic extra-planar gas layer can help us understand the origin of the gaseous Galactic halo and its interaction with the Milky Way disk. The 100-m Effelsberg radio telescope was utilized to detect and analyze a population of H
Autor:
L. Dedes, P.M.W. Kalberla
Publikováno v:
EAS Publications Series. 56:201-204
We derive the 3-D volume density distribution for the Milky Way H i gas out to a galactocentric distance R = 60 kpc and separate the extra-planar component from the disk gas. The main part of the Milky Way H i distribution is significantly warped but
Autor:
H. A. Ford, M. R. Calabretta, Brad K. Gibson, P. M. W. Kalberla, L. Dedes, Lister Staveley-Smith, Naomi McClure-Griffiths, Daniel J. Pisano, Jeremy Bailin, F. J. Lockman, Steven Janowiecki, K. Newton-McGee, Hiroyuki Nakanishi, Tara Murphy
Publikováno v:
The Astrophysical Journal Supplement Series. 181:398-412
The Parkes Galactic All-Sky Survey (GASS) is a survey of Galactic atomic hydrogen (HI) emission in the Southern sky covering declinations $\delta \leq 1^{\circ}$ using the Parkes Radio Telescope. The survey covers $2\pi$ steradians with an effective
Autor:
P. M. W. Kalberla, L. Dedes
Publikováno v:
Astronomy & Astrophysics. 487:951-963
Aims: We derive the 3-D HI volume density distribution for the Galactic disk out to R = 60 kpc. Methods: Our analysis is based on parameters for the warp and rotation curve derived previously. The data are taken from the Leiden/Argentine/Bonn all sky
Publikováno v:
Astronomy & Astrophysics. 469:511-527
Context. Gas within a galaxy is forced to establish pressure balance against gravitational forces. The shape of an unperturbed gaseous disk can be used to constrain dark matter models. Aims. We derive the 3-D HI volume density distribution for the Mi
The question, whether the stellar populations in the Milky Way take part in flaring of the scale heights as observed for the HI gas is a matter of debate. Standard mass models for the Milky Way assume a constant scale height for each of the different
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::abed89b2024eb2834012a5dad4de5e58
http://arxiv.org/abs/1408.5334
http://arxiv.org/abs/1408.5334
The discovery of an HI cloud with peculiar properties at equatorial coordinates (J2000) ra=07h49m, dec=04d30m is presented. The HI object was detected at 21cm using the 300-m NAIC Arecibo telescope. Subsequent follow-up high-resolution observations w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a2ef6b7d03a09a6da22370f8528b4fb
http://arxiv.org/abs/0810.3846
http://arxiv.org/abs/0810.3846
Autor:
L. Dedes, P. M. W. Kalberla
Publikováno v:
Mapping the Galaxy and Nearby Galaxies ISBN: 9780387727677
We investigate the disk-halo connection in the Milky Way and analyze the thick disk layer of HI gas which surrounds the Milky Way. To extract this part of the HI gas we determine first the global properties of the neutral gas disk. We use the Leiden/
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::465b1f7eccd445b1b4601fd002344b73
https://doi.org/10.1007/978-0-387-72768-4_53
https://doi.org/10.1007/978-0-387-72768-4_53
Autor:
Alyson Ford, Mark Calabretta, Daniel J. Pisano, Naomi McClure-Griffiths, Peter M. W. Kalberla, Brad K. Gibson, L. Dedes, Lister Staveley-Smith
Publikováno v:
ResearcherID
We present new high resolution neutral hydrogen (H I) images of the Galactic supershell GSH 242-03+37. These data were obtained with the Parkes Radiotelescope as part of the Galactic All-Sky Survey (GASS). GSH 242-03+37 is one of the largest and most
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b15fe339745f430d9156e5aaa8839103
http://arxiv.org/abs/astro-ph/0510304
http://arxiv.org/abs/astro-ph/0510304
Autor:
L. Dedes, Peter M. W. Kalberla
Publikováno v:
Proceedings of Baryons in Dark Matter Halos — PoS(BDMH2004).