Gas Kinematics in the Multiphase Circumgalactic Medium

Nikole M. Nielsen; Glenn G. Kacprzak; Christopher W. Churchill; Michael T. Murphy; Sowgat Muzahid; Jane C. Charlton; Jessica L. Evans

doi:10.1017/S1743921316011042

Gas Kinematics in the Multiphase Circumgalactic Medium

Nikole M. Nielsen, Glenn G. Kacprzak, Christopher W. Churchill, Michael T. Murphy, Sowgat Muzahid, Jane C. Charlton, Jessica L. Evans

Astronomy & Astrophysics

Research output: Contribution to journal › Article › peer-review

Abstract

We use high-resolution Keck, VLT, or Hubble Space Telescope spectra of background quasars to examine the kinematic properties of the multiphase, metal-enriched circumgalactic medium in the outskirts of galaxies at 0.08 < z gal < 1.0, focusing on the low-ionization Mgii and high-ionization Ovi doublets. The absorption kinematics of low-ionization gas in the circumgalactic medium depend strongly on the star formation activity and the location about the host galaxy, where the largest velocity dispersions are associated with blue, face-on galaxies probed along the minor axis. Conversely, high-ionization gas kinematics are independent of galaxy star formation activity and orientation.

Original language	English (US)
Pages (from-to)	345-347
Number of pages	3
Journal	Proceedings of the International Astronomical Union
Volume	11
Issue number	S321
DOIs	https://doi.org/10.1017/S1743921316011042
State	Published - Mar 1 2016

All Science Journal Classification (ASJC) codes

Medicine (miscellaneous)
Astronomy and Astrophysics
Nutrition and Dietetics
Public Health, Environmental and Occupational Health
Space and Planetary Science

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

Access to Document

10.1017/S1743921316011042

Cite this

@article{11fca034f41540b2b89bbc2b98b7d0e6,

title = "Gas Kinematics in the Multiphase Circumgalactic Medium",

abstract = "We use high-resolution Keck, VLT, or Hubble Space Telescope spectra of background quasars to examine the kinematic properties of the multiphase, metal-enriched circumgalactic medium in the outskirts of galaxies at 0.08 < z gal < 1.0, focusing on the low-ionization Mgii and high-ionization Ovi doublets. The absorption kinematics of low-ionization gas in the circumgalactic medium depend strongly on the star formation activity and the location about the host galaxy, where the largest velocity dispersions are associated with blue, face-on galaxies probed along the minor axis. Conversely, high-ionization gas kinematics are independent of galaxy star formation activity and orientation.",

author = "Nielsen, {Nikole M.} and Kacprzak, {Glenn G.} and Churchill, {Christopher W.} and Murphy, {Michael T.} and Sowgat Muzahid and Charlton, {Jane C.} and Evans, {Jessica L.}",

note = "Publisher Copyright: {\textcopyright} 2017 International Astronomical Union.",

year = "2016",

month = mar,

day = "1",

doi = "10.1017/S1743921316011042",

language = "English (US)",

volume = "11",

pages = "345--347",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

number = "S321",

}

TY - JOUR

T1 - Gas Kinematics in the Multiphase Circumgalactic Medium

AU - Nielsen, Nikole M.

AU - Kacprzak, Glenn G.

AU - Churchill, Christopher W.

AU - Murphy, Michael T.

AU - Muzahid, Sowgat

AU - Charlton, Jane C.

AU - Evans, Jessica L.

PY - 2016/3/1

Y1 - 2016/3/1

N2 - We use high-resolution Keck, VLT, or Hubble Space Telescope spectra of background quasars to examine the kinematic properties of the multiphase, metal-enriched circumgalactic medium in the outskirts of galaxies at 0.08 < z gal < 1.0, focusing on the low-ionization Mgii and high-ionization Ovi doublets. The absorption kinematics of low-ionization gas in the circumgalactic medium depend strongly on the star formation activity and the location about the host galaxy, where the largest velocity dispersions are associated with blue, face-on galaxies probed along the minor axis. Conversely, high-ionization gas kinematics are independent of galaxy star formation activity and orientation.

AB - We use high-resolution Keck, VLT, or Hubble Space Telescope spectra of background quasars to examine the kinematic properties of the multiphase, metal-enriched circumgalactic medium in the outskirts of galaxies at 0.08 < z gal < 1.0, focusing on the low-ionization Mgii and high-ionization Ovi doublets. The absorption kinematics of low-ionization gas in the circumgalactic medium depend strongly on the star formation activity and the location about the host galaxy, where the largest velocity dispersions are associated with blue, face-on galaxies probed along the minor axis. Conversely, high-ionization gas kinematics are independent of galaxy star formation activity and orientation.

UR - http://www.scopus.com/inward/record.url?scp=85046938176&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85046938176&partnerID=8YFLogxK

U2 - 10.1017/S1743921316011042

DO - 10.1017/S1743921316011042

M3 - Article

AN - SCOPUS:85046938176

SN - 1743-9213

VL - 11

SP - 345

EP - 347

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

IS - S321

ER -

Gas Kinematics in the Multiphase Circumgalactic Medium

Abstract

All Science Journal Classification (ASJC) codes

UN SDGs

Access to Document

Other files and links

Fingerprint

Cite this