語系:
繁體中文
English
說明(常見問題)
回圖書館首頁
手機版館藏查詢
登入
回首頁
切換:
標籤
|
MARC模式
|
ISBD
Applications of High-Resolution Obse...
~
Rosenfeld, Katherine.
FindBook
Google Book
Amazon
博客來
Applications of High-Resolution Observations at Millimeter Wavelengths.
紀錄類型:
書目-電子資源 : Monograph/item
正題名/作者:
Applications of High-Resolution Observations at Millimeter Wavelengths./
作者:
Rosenfeld, Katherine.
面頁冊數:
171 p.
附註:
Source: Dissertation Abstracts International, Volume: 77-09(E), Section: B.
Contained By:
Dissertation Abstracts International77-09B(E).
標題:
Astronomy. -
電子資源:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10102881
ISBN:
9781339665092
Applications of High-Resolution Observations at Millimeter Wavelengths.
Rosenfeld, Katherine.
Applications of High-Resolution Observations at Millimeter Wavelengths.
- 171 p.
Source: Dissertation Abstracts International, Volume: 77-09(E), Section: B.
Thesis (Ph.D.)--Harvard University, 2016.
Interferometric observations at millimeter wavelengths provide a precious, detailed view of certain astrophysical objects. This thesis is composed of studies that both rely on and enable this technique to study the structure of planet-forming disks and soon image the closest regions around super-massive black holes. Young stars form out of a cloud of gas and dust that, before its eventual dissipation, flattens to a disk. However the disk population is diverse and recent high-resolution images have revealed a wide variety of interesting features. To understand these observations we use detailed radiative transfer models to motivate various physical scenarios. First we identify a set of traits in the disk around V4046 Sgr that marks the coupled progression of the gas and dust distributions in the presence of at least one embedded companion. Next, we investigate how the vertical temperature structure of a disk can be spatially resolved and apply our framework to observations of the disk around HD163296. Lastly, we show how large-scale radial flows of gas may be observable and question how this phenomenon might be distinguished from other scenarios such as warps or outflows. The last chapter summarizes the APHIDS project which changes the sampling rate of data taken at the SMA so that it may be used for VLBI campaigns.
ISBN: 9781339665092Subjects--Topical Terms:
517668
Astronomy.
Applications of High-Resolution Observations at Millimeter Wavelengths.
LDR
:02198nmm a2200265 4500
001
2078996
005
20161128143922.5
008
170521s2016 ||||||||||||||||| ||eng d
020
$a
9781339665092
035
$a
(MiAaPQ)AAI10102881
035
$a
AAI10102881
040
$a
MiAaPQ
$c
MiAaPQ
100
1
$a
Rosenfeld, Katherine.
$3
3194642
245
1 0
$a
Applications of High-Resolution Observations at Millimeter Wavelengths.
300
$a
171 p.
500
$a
Source: Dissertation Abstracts International, Volume: 77-09(E), Section: B.
500
$a
Advisers: Karin I. Oberg; Sean M. Andrews.
502
$a
Thesis (Ph.D.)--Harvard University, 2016.
520
$a
Interferometric observations at millimeter wavelengths provide a precious, detailed view of certain astrophysical objects. This thesis is composed of studies that both rely on and enable this technique to study the structure of planet-forming disks and soon image the closest regions around super-massive black holes. Young stars form out of a cloud of gas and dust that, before its eventual dissipation, flattens to a disk. However the disk population is diverse and recent high-resolution images have revealed a wide variety of interesting features. To understand these observations we use detailed radiative transfer models to motivate various physical scenarios. First we identify a set of traits in the disk around V4046 Sgr that marks the coupled progression of the gas and dust distributions in the presence of at least one embedded companion. Next, we investigate how the vertical temperature structure of a disk can be spatially resolved and apply our framework to observations of the disk around HD163296. Lastly, we show how large-scale radial flows of gas may be observable and question how this phenomenon might be distinguished from other scenarios such as warps or outflows. The last chapter summarizes the APHIDS project which changes the sampling rate of data taken at the SMA so that it may be used for VLBI campaigns.
590
$a
School code: 0084.
650
4
$a
Astronomy.
$3
517668
690
$a
0606
710
2
$a
Harvard University.
$b
Astronomy.
$3
3173874
773
0
$t
Dissertation Abstracts International
$g
77-09B(E).
790
$a
0084
791
$a
Ph.D.
792
$a
2016
793
$a
English
856
4 0
$u
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10102881
筆 0 讀者評論
館藏地:
全部
電子資源
出版年:
卷號:
館藏
1 筆 • 頁數 1 •
1
條碼號
典藏地名稱
館藏流通類別
資料類型
索書號
使用類型
借閱狀態
預約狀態
備註欄
附件
W9311864
電子資源
11.線上閱覽_V
電子書
EB
一般使用(Normal)
在架
0
1 筆 • 頁數 1 •
1
多媒體
評論
新增評論
分享你的心得
Export
取書館
處理中
...
變更密碼
登入
(1)帳號:一般為「身分證號」;外籍生或交換生則為「學號」。 (2)密碼:預設為帳號末四碼。
帳號
.
密碼
.
請在此電腦上記得個人資料
取消
忘記密碼? (請注意!您必須已在系統登記E-mail信箱方能使用。)