語系:
繁體中文
English
說明(常見問題)
登入
回首頁
切換:
標籤
|
MARC模式
|
ISBD
Lyman-alpha as an Astrophysical and ...
~
Dijkstra, Mark.
Lyman-alpha as an Astrophysical and Cosmological Tool = Saas-Fee Advanced Course 46. Swiss Society for Astrophysics and Astronomy /
紀錄類型:
書目-語言資料,印刷品 : Monograph/item
正題名/作者:
Lyman-alpha as an Astrophysical and Cosmological Tool/ by Mark Dijkstra, J. Xavier Prochaska, Masami Ouchi, Matthew Hayes ; edited by Anne Verhamme, Pierre North, Sebastiano Cantalupo, Hakim Atek.
其他題名:
Saas-Fee Advanced Course 46. Swiss Society for Astrophysics and Astronomy /
作者:
Dijkstra, Mark.
其他作者:
Prochaska, J. Xavier.
面頁冊數:
XVII, 403 p. 313 illus., 192 illus. in color.online resource. :
Contained By:
Springer Nature eBook
標題:
Observations, Astronomical. -
電子資源:
https://doi.org/10.1007/978-3-662-59623-4
ISBN:
9783662596234
Lyman-alpha as an Astrophysical and Cosmological Tool = Saas-Fee Advanced Course 46. Swiss Society for Astrophysics and Astronomy /
Dijkstra, Mark.
Lyman-alpha as an Astrophysical and Cosmological Tool
Saas-Fee Advanced Course 46. Swiss Society for Astrophysics and Astronomy /[electronic resource] :by Mark Dijkstra, J. Xavier Prochaska, Masami Ouchi, Matthew Hayes ; edited by Anne Verhamme, Pierre North, Sebastiano Cantalupo, Hakim Atek. - 1st ed. 2019. - XVII, 403 p. 313 illus., 192 illus. in color.online resource. - Saas-Fee Advanced Course,461861-7980 ;. - Saas-Fee Advanced Course,42.
Physics of Lya Radiative Transfer -- HI Absorption in the Intergalactic Medium -- Observations of Lya Emitters at High Redshift -- Lyman alpha Emission and Absorption in Local Galaxies -- Index. .
The hydrogen Lyman-alpha line is of utmost importance to many fields of astrophysics. This UV line being conveniently redshifted with distance to the visible and even near infrared wavelength ranges, it is observable from the ground, and provides the main observational window on the formation and evolution of high redshift galaxies. Absorbing systems that would otherwise go unnoticed are revealed through the Lyman-alpha forest, Lyman-limit, and damped Lyman-alpha systems, tracing the distribution of baryonic matter on large scales, and its chemical enrichment. We are living an exciting epoch with the advent of new instruments and facilities, on board of satellites and on the ground. Wide field and very sensitive integral field spectrographs are becoming available on the ground, such as MUSE at the ESO VLT. The giant E-ELT and TMT telescopes will foster a quantum leap in sensitivity and both spatial and spectroscopic resolution, to the point of being able, perhaps, to measure directly the acceleration of the Hubble flow. In space, the JWST will open new possibilities to study the Lyman-alpha emission of primordial galaxies in the near infrared. As long as the Hubble Space Telescope will remain available, the UV-restframe properties of nearby galaxies will be accessible to our knowledge. Therefore, this Saas-Fee course appears very timely and should meet the interest of many young researchers.
ISBN: 9783662596234
Standard No.: 10.1007/978-3-662-59623-4doiSubjects--Topical Terms:
1254353
Observations, Astronomical.
LC Class. No.: QB4
Dewey Class. No.: 520
Lyman-alpha as an Astrophysical and Cosmological Tool = Saas-Fee Advanced Course 46. Swiss Society for Astrophysics and Astronomy /
LDR
:03219nam a22004095i 4500
001
1006749
003
DE-He213
005
20200630075034.0
007
cr nn 008mamaa
008
210106s2019 gw | s |||| 0|eng d
020
$a
9783662596234
$9
978-3-662-59623-4
024
7
$a
10.1007/978-3-662-59623-4
$2
doi
035
$a
978-3-662-59623-4
050
4
$a
QB4
072
7
$a
PG
$2
bicssc
072
7
$a
SCI004000
$2
bisacsh
072
7
$a
PG
$2
thema
082
0 4
$a
520
$2
23
100
1
$a
Dijkstra, Mark.
$e
author.
$4
aut
$4
http://id.loc.gov/vocabulary/relators/aut
$3
1300374
245
1 0
$a
Lyman-alpha as an Astrophysical and Cosmological Tool
$h
[electronic resource] :
$b
Saas-Fee Advanced Course 46. Swiss Society for Astrophysics and Astronomy /
$c
by Mark Dijkstra, J. Xavier Prochaska, Masami Ouchi, Matthew Hayes ; edited by Anne Verhamme, Pierre North, Sebastiano Cantalupo, Hakim Atek.
250
$a
1st ed. 2019.
264
1
$a
Berlin, Heidelberg :
$b
Springer Berlin Heidelberg :
$b
Imprint: Springer,
$c
2019.
300
$a
XVII, 403 p. 313 illus., 192 illus. in color.
$b
online resource.
336
$a
text
$b
txt
$2
rdacontent
337
$a
computer
$b
c
$2
rdamedia
338
$a
online resource
$b
cr
$2
rdacarrier
347
$a
text file
$b
PDF
$2
rda
490
1
$a
Saas-Fee Advanced Course,
$x
1861-7980 ;
$v
46
505
0
$a
Physics of Lya Radiative Transfer -- HI Absorption in the Intergalactic Medium -- Observations of Lya Emitters at High Redshift -- Lyman alpha Emission and Absorption in Local Galaxies -- Index. .
520
$a
The hydrogen Lyman-alpha line is of utmost importance to many fields of astrophysics. This UV line being conveniently redshifted with distance to the visible and even near infrared wavelength ranges, it is observable from the ground, and provides the main observational window on the formation and evolution of high redshift galaxies. Absorbing systems that would otherwise go unnoticed are revealed through the Lyman-alpha forest, Lyman-limit, and damped Lyman-alpha systems, tracing the distribution of baryonic matter on large scales, and its chemical enrichment. We are living an exciting epoch with the advent of new instruments and facilities, on board of satellites and on the ground. Wide field and very sensitive integral field spectrographs are becoming available on the ground, such as MUSE at the ESO VLT. The giant E-ELT and TMT telescopes will foster a quantum leap in sensitivity and both spatial and spectroscopic resolution, to the point of being able, perhaps, to measure directly the acceleration of the Hubble flow. In space, the JWST will open new possibilities to study the Lyman-alpha emission of primordial galaxies in the near infrared. As long as the Hubble Space Telescope will remain available, the UV-restframe properties of nearby galaxies will be accessible to our knowledge. Therefore, this Saas-Fee course appears very timely and should meet the interest of many young researchers.
650
0
$a
Observations, Astronomical.
$3
1254353
650
0
$a
Astronomy—Observations.
$3
1254354
650
0
$a
Cosmology.
$3
579761
650
0
$a
Astrophysics.
$3
646223
650
1 4
$a
Astronomy, Observations and Techniques.
$3
769023
650
2 4
$a
Astrophysics and Astroparticles.
$3
782546
700
1
$a
Prochaska, J. Xavier.
$e
author.
$4
aut
$4
http://id.loc.gov/vocabulary/relators/aut
$3
1300375
700
1
$a
Ouchi, Masami.
$e
author.
$4
aut
$4
http://id.loc.gov/vocabulary/relators/aut
$3
1300376
700
1
$a
Hayes, Matthew.
$e
author.
$4
aut
$4
http://id.loc.gov/vocabulary/relators/aut
$3
1300377
700
1
$a
Verhamme, Anne.
$e
editor.
$4
edt
$4
http://id.loc.gov/vocabulary/relators/edt
$3
1300378
700
1
$a
North, Pierre.
$e
editor.
$4
edt
$4
http://id.loc.gov/vocabulary/relators/edt
$3
1300379
700
1
$a
Cantalupo, Sebastiano.
$e
editor.
$4
edt
$4
http://id.loc.gov/vocabulary/relators/edt
$3
1300380
700
1
$a
Atek, Hakim.
$e
editor.
$4
edt
$4
http://id.loc.gov/vocabulary/relators/edt
$3
1300381
710
2
$a
SpringerLink (Online service)
$3
593884
773
0
$t
Springer Nature eBook
776
0 8
$i
Printed edition:
$z
9783662596227
776
0 8
$i
Printed edition:
$z
9783662596241
776
0 8
$i
Printed edition:
$z
9783662596258
830
0
$a
Saas-Fee Advanced Course,
$x
1861-7980 ;
$v
42
$3
1258909
856
4 0
$u
https://doi.org/10.1007/978-3-662-59623-4
912
$a
ZDB-2-PHA
912
$a
ZDB-2-SXP
950
$a
Physics and Astronomy (SpringerNature-11651)
950
$a
Physics and Astronomy (R0) (SpringerNature-43715)
筆 0 讀者評論
多媒體
評論
新增評論
分享你的心得
Export
取書館別
處理中
...
變更密碼[密碼必須為2種組合(英文和數字)及長度為10碼以上]
登入