Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Suzanne M. Linder"'
Autor:
Jonathan Ivor Davies, Suzanne M. Linder, Rhodri Evans, Roland Gunesch, Sabina Sabatini, Rodney Smith, Maarten Baes, Sarah Roberts
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 342:1093-1101
Some Lyman continuum photons are likely to escape from most galaxies, and these can play an important role in ionizing gas around and between galaxies, including gas that gives rise to Lyman alpha absorption. Thus the gas surrounding galaxies and in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::934e42e7575697f44b02daa9b7f2a95b
https://doi.org/10.1046/j.1365-8711.2003.06625.x
https://doi.org/10.1046/j.1365-8711.2003.06625.x
Autor:
S. Roberts, Rhodri Evans, Jonathan Ivor Davies, Luke J. M. Davies, Rodney Smith, Suzanne M. Linder, Sabina Sabatini
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 336:155-158
It has been suggested that some high-velocity hydrogen clouds, rather than being associated with the Galaxy, may be dispersed throughout the Local Group. If true these hydrogen clouds may be the ‘debris’ left over from the formation of the Local
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5baad7882623709018f0dfa8655b0472
https://doi.org/10.1046/j.1365-8711.2002.05711.x
https://doi.org/10.1046/j.1365-8711.2002.05711.x
Autor:
Suzanne M. Linder
Publikováno v:
The Astrophysical Journal. 529:644-654
The effects of galaxy selection on our ability to constrain the nature of weak Ly\alpha absorbers at low redshift are explored. Current observations indicate the existence of a population of gas-rich, low surface brightness (LSB) galaxies, and these
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a3d666d1f8b4372cd43e2346d9e5ae61
https://doi.org/10.1086/308319
https://doi.org/10.1086/308319
Autor:
Suzanne M. Linder
Publikováno v:
International Astronomical Union Colloquium. 171:323-330
Using simulations of the low redshift galaxy population based upon galaxy observations, it is shown (Linder 1998) that the majority of Lyα absorbers at low redshift could arise in low surface brightness (LSB) galaxies. The contribution to absorption
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3859cdfcb4a3dc385b21a9b1ad1ce54b
https://doi.org/10.1017/s0252921100054506
https://doi.org/10.1017/s0252921100054506
Autor:
Suzanne M. Linder
Publikováno v:
The Astrophysical Journal. 495:637-646
A scenario is explored in which Lyman alpha absorbers at low redshift arise from lines of sight through extended galaxy disks, including those of dwarf and low surface brightness galaxies. A population of galaxies is simulated based upon observed dis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f7e627719a58c235687aac864a3f94a6
https://doi.org/10.1086/305332
https://doi.org/10.1086/305332
Publikováno v:
AIP Conference Proceedings.
Numerous studies suggest that stronger Lyα absorbers are more closely associated with galaxies, while weaker absorbers arise in the intragroup medium surrounding concentrations of galaxies near the absorber redshift. What can absorbers tell us about
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a43d47891a8be7dd533c9d32a77c51a5
https://doi.org/10.1063/1.2973589
https://doi.org/10.1063/1.2973589
Autor:
Suzanne M. Linder
Publikováno v:
AIP Conference Proceedings.
If a few percent of ionizing ultraviolet photons escape from galaxies, then normal galaxies make a modest (30 to 40 percent) and spatially varying contribution to the ionizing background at low redshift (Linder et al.). Supposing that galaxies form w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::349c59f347438c96515895bead5499d8
https://doi.org/10.1063/1.1913964
https://doi.org/10.1063/1.1913964
Autor:
Jonathan Ivor Davies, S. Roberts, Rhodri Evans, Rodney Smith, Maarten Baes, Robert F. Minchin, Suzanne M. Linder, Sabina Sabatini
The HIDEEP survey (Minchin et al. 2003) was done in an attempt to find objects having low inferred neutral hydrogen column densities, yet they found a distribution which was strongly peaked at 10^20.65 cm^-2. In an attempt to understand this distribu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38883403abec44ec3c0ab432d5e0ef59
http://arxiv.org/abs/astro-ph/0405477
http://arxiv.org/abs/astro-ph/0405477
Autor:
Sabina Sabatini, Rhodri Evans, Jonathan Ivor Davies, Suzanne M. Linder, Herwig Dejonghe, W. J. G. de Blok, Sarah Roberts, Maarten Baes, Rodney Smith
We present SKIRT (Stellar Kinematics Including Radiative Transfer), a new Monte Carlo radiative transfer code that allows the calculation of the observed stellar kinematics of a dusty galaxy. The code incorporates the effects of both absorption and s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c450b09ef6c29ac2a291deffbca2d08
Autor:
Suzanne M. Linder
Publikováno v:
Astrophysics and Space Science Library ISBN: 9789401039789
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a1ff22bdee3812a8c88ce09ebb8373c4
https://doi.org/10.1007/978-94-010-0115-1_11
https://doi.org/10.1007/978-94-010-0115-1_11