Journal articles
The structure of the local hot bubble
Wenhao Liu
1
Meng Chiao
2
Michael R. Collier
2
Thomas Cravens
3
Massimiliano Galeazzi
1
Dimitra Koutroumpa
4
Kip D. Kuntz
5
Rosine Lallement
6
Susan T. Lepri
7
Dan Mccammon
8
Kelsey Morgan
8
Frederick Scott Porter
2
Steven L. Snowden
2
Nicholas Evan Thomas
2
Youaraj Uprety
1, 9
Eugenio Ursino
1, 10
Brian Walsh
11
Massimiliano Galeazzi 1
Author
Dimitra Koutroumpa 4
Author IdHAL : dimitra-koutroumpa ORCID : https://orcid.org/0000-0002-5716-3412
Kip D. Kuntz 5
Author
Rosine Lallement 6
Author
Susan T. Lepri 7
Author
Dan Mccammon 8
Author
Kelsey Morgan 8
Author
Frederick Scott Porter 2
Author
Steven L. Snowden 2
Author
Nicholas Evan Thomas 2
Author
Youaraj Uprety 1, 9
Author
Eugenio Ursino 1, 10
Author
Brian Walsh 11
Author
1
Department of Physics [Coral Gables] (Coral Gables, FL 33124 - United States)
- University of Miami [Coral Gables] ( 1320 S Dixie Hwy, Coral Gables, FL 33146 - United States)
2
GSFC - NASA Goddard Space Flight Center (Greenbelt, MD 20771 - United States)
3
Department of Physics and Astronomy [Lawrence Kansas] (1082 Malott,1251 Wescoe Hall Dr., Lawrence, KS 66045-758 - United States)
- KU - University of Kansas [Lawrence] (1450 Jayhawk Blvd, Lawrence, KS 66045 - United States)
4
HEPPI - LATMOS (France)
- LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales (11 boulevard d'Alembert
Quartier des Garennes
78280 - Guyancourt - France)
- UVSQ - Université de Versailles Saint-Quentin-en-Yvelines : UMR8190 (55 avenue de Paris - 78035 Versailles cedex - France)
- UPMC - Université Pierre et Marie Curie - Paris 6 : UMR8190 (4 place Jussieu - 75005 Paris - France)
- INSU - CNRS - Institut national des sciences de l'Univers : UMR8190 (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8190 (France)
5
Department of Physics and Astronomy [Baltimore] (3400 North Charles Street, Baltimore, MD 21218 - United States)
- JHU - Johns Hopkins University (Baltimore, Maryland 410-516-8000 - United States)
6
GEPI - Galaxies, Etoiles, Physique, Instrumentation (5, place Jules Janssen 92195 MEUDON CEDEX - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- UPD7 - Université Paris Diderot - Paris 7 : UMR_8111 (5 rue Thomas-Mann - 75205 Paris cedex 13 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_8111 (France)
7
AOSS - Department of Atmospheric, Oceanic, and Space Sciences [Ann Arbor] (Ann Arbor, MI 48109 - United States)
- University of Michigan [Ann Arbor] (500 Church Street Ann Arbor, MI 48109-1090 - United States)
- University of Michigan System (Michigan - United States)
8
Department of Physics [Madison] (1150 University Avenue,
Madison, WI 53706-1390 - United States)
- University of Wisconsin-Madison (Madison, WI 53706 - United States)
9
Department of Physics and Astronomy [Murfreesboro] (Murfreesboro, TN - United States)
- MTSU - Middle Tennessee State University [Murfreesboro] (1301 East Main Street, Murfreesboro, TN 37132-0001 - United States)
10
Department of Physics [Grinnell] (1116 8th Avenue, Grinnell, IA 50112 - United States)
- Grinnell College (1115 8th Avenue, Grinnell, IA50112 - United States)
11
Department of Mechanical Engineering [Boston] (College of Engineering, 110 Cummington Mall, Boston MA 02215 - United States)
- BU - Boston University [Boston] (One Silber Way, Boston, MA 02215 - United States)
Abstract : DXL (Diffuse X-rays from the Local Galaxy) is a sounding rocket mission designed to quantify and characterize the contribution of Solar Wind Charge eXchange (SWCX) to the Diffuse X-ray Background and study the properties of the Local Hot Bubble (LHB). Based on the results from the DXL mission, we quantified and removed the contribution of SWCX to the diffuse X-ray background measured by the ROSAT All Sky Survey (RASS). The "cleaned" maps were used to investigate the physical properties of the LHB. Assuming thermal ionization equilibrium, we measured a highly uniform temperature distributed around kT=0.097 keV+/-0.013 keV (FWHM)+/-0.006 keV (systematic). We also generated a thermal emission measure map and used it to characterize the three-dimensional (3D) structure of the LHB which we found to be in good agreement with the structure of the local cavity measured from dust and gas.
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Journal articles
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https://hal-insu.archives-ouvertes.fr/insu-01399545
Contributor : Catherine Cardon <>
Submitted on : Friday, November 27, 2020 - 6:35:44 PM
Last modification on : Monday, December 14, 2020 - 12:21:20 PM
Contributor : Catherine Cardon <>
Submitted on : Friday, November 27, 2020 - 6:35:44 PM
Last modification on : Monday, December 14, 2020 - 12:21:20 PM
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Identifiers
- HAL Id : insu-01399545, version 1
- ARXIV : 1611.05133
- BIBCODE : 2016arXiv161105133L
- DOI : 10.3847/1538-4357/834/1/33
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Citation
Wenhao Liu, Meng Chiao, Michael R. Collier, Thomas Cravens, Massimiliano Galeazzi, et al.. The structure of the local hot bubble. The Astrophysical Journal, American Astronomical Society, 2017, 834 (1), pp.art. 33. ⟨10.3847/1538-4357/834/1/33⟩. ⟨insu-01399545⟩
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