Language:
English
繁體中文
Help
回圖書館首頁
手機版館藏查詢
Login
Back
Switch To:
Labeled
|
MARC Mode
|
ISBD
Linked to FindBook
Google Book
Amazon
博客來
ELVES and Dwarfs : = Elucidating Low-Mass Galaxies with the Exploration of Local VolumE Satellites Survey.
Record Type:
Electronic resources : Monograph/item
Title/Author:
ELVES and Dwarfs :/
Reminder of title:
Elucidating Low-Mass Galaxies with the Exploration of Local VolumE Satellites Survey.
Author:
Carlsten, Scott.
Description:
1 online resource (468 pages)
Notes:
Source: Dissertations Abstracts International, Volume: 84-04, Section: B.
Contained By:
Dissertations Abstracts International84-04B.
Subject:
Astrophysics. -
Online resource:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=29211515click for full text (PQDT)
ISBN:
9798351480633
ELVES and Dwarfs : = Elucidating Low-Mass Galaxies with the Exploration of Local VolumE Satellites Survey.
Carlsten, Scott.
ELVES and Dwarfs :
Elucidating Low-Mass Galaxies with the Exploration of Local VolumE Satellites Survey. - 1 online resource (468 pages)
Source: Dissertations Abstracts International, Volume: 84-04, Section: B.
Thesis (Ph.D.)--Princeton University, 2022.
Includes bibliographical references
Low-mass, "dwarf" galaxies are ubiquitous probes of dark matter and galaxy formation physics. Many are found as satellites of more massive galaxies, like the Milky Way (MW). In fact, the dwarf satellites of the MW have long been a central observational benchmark for models of small-scale structure formation and dwarf evolution. However, it is critical to move beyond just the MW and consider the dwarf satellites of a statistically large sample of host galaxies. To do this, I developed the Exploration of Local VolumE Satellites (ELVES) Survey, which characterized the dwarf satellites of a volume-limited sample of 30 nearby massive, MW-like hosts.Progressing this survey involved developing specialized detection algorithms to find these faint galaxies and sophisticated distance measurement techniques to constrain the distances of the detections. This is important to confirm that the detected galaxies are actually satellites of a certain host and not contaminants along the line of sight. The end result is a census of the "classical" (i.e. M* ≳ 105.5 M⊙) satellites of 30 hosts, roughly a 5x increase over the statistics previously available.With this expanded sample of hosts, I compared the observed satellite abundance to that predicted from galaxy formation models, finding good agreement. The observed satellite spatial distribution did not, however, agree well with predictions from current models. In terms of satellite abundance and spatial distribution, the MW appears remarkably typical among comparable systems. I performed an in-depth investigation into the structure of dwarf satellites and quantified various scaling relations that will be useful benchmarks for future galaxy formation simulations. Finally, I investigated the star cluster properties of these dwarf galaxies, uncovering an interesting dependence on the large-scale environment that the dwarf resides in. The survey presents a unique dataset that can be used to explore various other aspects of near-field cosmology and dwarf evolution.
Electronic reproduction.
Ann Arbor, Mich. :
ProQuest,
2023
Mode of access: World Wide Web
ISBN: 9798351480633Subjects--Topical Terms:
535904
Astrophysics.
Subjects--Index Terms:
Dwarf galaxiesIndex Terms--Genre/Form:
542853
Electronic books.
ELVES and Dwarfs : = Elucidating Low-Mass Galaxies with the Exploration of Local VolumE Satellites Survey.
LDR
:03356nmm a2200361K 4500
001
2363314
005
20231121104605.5
006
m o d
007
cr mn ---uuuuu
008
241011s2022 xx obm 000 0 eng d
020
$a
9798351480633
035
$a
(MiAaPQ)AAI29211515
035
$a
AAI29211515
040
$a
MiAaPQ
$b
eng
$c
MiAaPQ
$d
NTU
100
1
$a
Carlsten, Scott.
$3
3704073
245
1 0
$a
ELVES and Dwarfs :
$b
Elucidating Low-Mass Galaxies with the Exploration of Local VolumE Satellites Survey.
264
0
$c
2022
300
$a
1 online resource (468 pages)
336
$a
text
$b
txt
$2
rdacontent
337
$a
computer
$b
c
$2
rdamedia
338
$a
online resource
$b
cr
$2
rdacarrier
500
$a
Source: Dissertations Abstracts International, Volume: 84-04, Section: B.
500
$a
Advisor: Greene, Jenny E.
502
$a
Thesis (Ph.D.)--Princeton University, 2022.
504
$a
Includes bibliographical references
520
$a
Low-mass, "dwarf" galaxies are ubiquitous probes of dark matter and galaxy formation physics. Many are found as satellites of more massive galaxies, like the Milky Way (MW). In fact, the dwarf satellites of the MW have long been a central observational benchmark for models of small-scale structure formation and dwarf evolution. However, it is critical to move beyond just the MW and consider the dwarf satellites of a statistically large sample of host galaxies. To do this, I developed the Exploration of Local VolumE Satellites (ELVES) Survey, which characterized the dwarf satellites of a volume-limited sample of 30 nearby massive, MW-like hosts.Progressing this survey involved developing specialized detection algorithms to find these faint galaxies and sophisticated distance measurement techniques to constrain the distances of the detections. This is important to confirm that the detected galaxies are actually satellites of a certain host and not contaminants along the line of sight. The end result is a census of the "classical" (i.e. M* ≳ 105.5 M⊙) satellites of 30 hosts, roughly a 5x increase over the statistics previously available.With this expanded sample of hosts, I compared the observed satellite abundance to that predicted from galaxy formation models, finding good agreement. The observed satellite spatial distribution did not, however, agree well with predictions from current models. In terms of satellite abundance and spatial distribution, the MW appears remarkably typical among comparable systems. I performed an in-depth investigation into the structure of dwarf satellites and quantified various scaling relations that will be useful benchmarks for future galaxy formation simulations. Finally, I investigated the star cluster properties of these dwarf galaxies, uncovering an interesting dependence on the large-scale environment that the dwarf resides in. The survey presents a unique dataset that can be used to explore various other aspects of near-field cosmology and dwarf evolution.
533
$a
Electronic reproduction.
$b
Ann Arbor, Mich. :
$c
ProQuest,
$d
2023
538
$a
Mode of access: World Wide Web
650
4
$a
Astrophysics.
$3
535904
653
$a
Dwarf galaxies
653
$a
Galaxies
653
$a
Groups of galaxies
653
$a
Observational astronomy
655
7
$a
Electronic books.
$2
lcsh
$3
542853
690
$a
0596
710
2
$a
ProQuest Information and Learning Co.
$3
783688
710
2
$a
Princeton University.
$b
Astrophysical Sciences.
$3
3193121
773
0
$t
Dissertations Abstracts International
$g
84-04B.
856
4 0
$u
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=29211515
$z
click for full text (PQDT)
based on 0 review(s)
Location:
ALL
電子資源
Year:
Volume Number:
Items
1 records • Pages 1 •
1
Inventory Number
Location Name
Item Class
Material type
Call number
Usage Class
Loan Status
No. of reservations
Opac note
Attachments
W9485670
電子資源
11.線上閱覽_V
電子書
EB
一般使用(Normal)
On shelf
0
1 records • Pages 1 •
1
Multimedia
Reviews
Add a review
and share your thoughts with other readers
Export
pickup library
Processing
...
Change password
Login