Zobrazeno 1 - 10
of 33
pro vyhledávání: '"P. M. W. Kalberla"'
Context. There are significant amounts of H2 in the Milky Way. Due to its symmetry H2 does not radiate at radio frequencies. CO is thought to be a tracer for H2, however CO is formed at significantly higher opacities than H2. Thus, toward high Galact
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::25000be5e77061eaea8fc82c65aede72
http://arxiv.org/abs/2004.14630
http://arxiv.org/abs/2004.14630
Publikováno v:
Astronomy & Astrophysics. 654:A91
Context. H I filaments are closely related to dusty magnetized structures that are observable in the far infrared (FIR). Recently it was proposed that the coherence of oriented H I structures in velocity traces the line of sight magnetic field tangli
Publikováno v:
The Astronomical journal (N.Y.N.Y.) 157 (2019). doi:10.3847/1538-3881/aaf3b3
info:cnr-pdr/source/autori:Lopez-Corredoira M.; Sylos Labini F.; Kalberla P.M.W.; Allende Prieto C./titolo:Radial Velocities in the Outermost Disk toward the Anticenter/doi:10.3847%2F1538-3881%2Faaf3b3/rivista:The Astronomical journal (N.Y.N.Y.)/anno:2019/pagina_da:/pagina_a:/intervallo_pagine:/volume:157
info:cnr-pdr/source/autori:Lopez-Corredoira M.; Sylos Labini F.; Kalberla P.M.W.; Allende Prieto C./titolo:Radial Velocities in the Outermost Disk toward the Anticenter/doi:10.3847%2F1538-3881%2Faaf3b3/rivista:The Astronomical journal (N.Y.N.Y.)/anno:2019/pagina_da:/pagina_a:/intervallo_pagine:/volume:157
We measure the mean Galactocentric radial component of the velocity of stars ($v_R$) in the disk at 8 kpc$17$ kpc. Negative velocities are also observed in 21 cm HI maps, possibly dominated by local gas emission. Among the possible dynamical causes f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54b2404a2378f377458eab163fca6e77
http://www.cnr.it/prodotto/i/399044
http://www.cnr.it/prodotto/i/399044
Autor:
P. M. W. Kalberla, J. Kerp
The local Galactic HI gas was found to contain cold neutral medium (CNM) filaments that are aligned with polarized dust emission. These filaments appear to be dominated by the magnetic field and in this case turbulence is expected to show distinct an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::50f8410f9033f9c467244dca73e9fb69
http://arxiv.org/abs/1608.05369
http://arxiv.org/abs/1608.05369
The subsequent coalescence of low--mass halos over cosmic time is thought to be the major formation channel of massive spiral galaxies like the Milky Way and the Andromeda Galaxy (M31). The gaseous halo of a massive galaxy is considered to be the res
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f0427fd728948bf14228db5e539b01f
Autor:
Urmas Haud, P. M. W. Kalberla
Publikováno v:
Astronomy & Astrophysics. 619:A58
Context. A large fraction of the interstellar medium can be characterized as a multiphase medium. The neutral hydrogen gas is bistable with a cold and warm neutral medium (CNM and WNM respectively) but there is evidence for an additional phase at int
Publikováno v:
The Astrophysical Journal Supplement Series. 188:488-499
Starting in winter 2008/2009 an L-band 7-Feed-Array receiver is used for a 21-cm line survey performed with the 100-m telescope, the Effelsberg-Bonn HI survey (EBHIS). The EBHIS will cover the whole northern hemisphere for decl.>-5 deg comprising bot
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
Autor:
P. M. W. Kalberla, Urmas Haud
Publikováno v:
Astronomy & Astrophysics. 466:555-564
Aims. We investigate the properties of the 21-cm radio-lines of galactic neutral hydrogen by decomposing, the profiles of "The Leiden/Argentine/Bonn (LAB) Survey of Galactic H I" into Gaussian components. The width distribution of the obtained compon