Soft X-Ray background flux

A. N. Bunner; P. C. Coleman; W. L. Kraushaar; D. McCammon; T. M. Palmieri; A. Shilepsky; M. Ulmer

doi:10.1038/2231222a0

Soft X-Ray background flux

A. N. Bunner^*, P. C. Coleman, W. L. Kraushaar, D. McCammon, T. M. Palmieri, A. Shilepsky, M. Ulmer

^*Corresponding author for this work

Physics and Astronomy

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

45 Scopus citations

Abstract

Measurements of the soft X-ray background flux show good qualitative correlation with 21 cm measurements of columnar hydrogen density but too little apparent absorption. A portion of the flux may originate in unresolved population II objects or may be extragalactic.

Original language	English (US)
Pages (from-to)	1222-1226
Number of pages	5
Journal	Nature
Volume	223
Issue number	5212
DOIs	https://doi.org/10.1038/2231222a0
State	Published - Dec 1 1969

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@article{9f41716029ee4d52b5f603a8123435dc,

title = "Soft X-Ray background flux",

abstract = "Measurements of the soft X-ray background flux show good qualitative correlation with 21 cm measurements of columnar hydrogen density but too little apparent absorption. A portion of the flux may originate in unresolved population II objects or may be extragalactic.",

author = "Bunner, {A. N.} and Coleman, {P. C.} and Kraushaar, {W. L.} and D. McCammon and Palmieri, {T. M.} and A. Shilepsky and M. Ulmer",

year = "1969",

month = dec,

day = "1",

doi = "10.1038/2231222a0",

language = "English (US)",

volume = "223",

pages = "1222--1226",

journal = "Nature",

issn = "0028-0836",

publisher = "Nature Publishing Group",

number = "5212",

}

TY - JOUR

T1 - Soft X-Ray background flux

AU - Bunner, A. N.

AU - Coleman, P. C.

AU - Kraushaar, W. L.

AU - McCammon, D.

AU - Palmieri, T. M.

AU - Shilepsky, A.

AU - Ulmer, M.

PY - 1969/12/1

Y1 - 1969/12/1

N2 - Measurements of the soft X-ray background flux show good qualitative correlation with 21 cm measurements of columnar hydrogen density but too little apparent absorption. A portion of the flux may originate in unresolved population II objects or may be extragalactic.

AB - Measurements of the soft X-ray background flux show good qualitative correlation with 21 cm measurements of columnar hydrogen density but too little apparent absorption. A portion of the flux may originate in unresolved population II objects or may be extragalactic.

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UR - http://www.scopus.com/inward/citedby.url?scp=0041426831&partnerID=8YFLogxK

U2 - 10.1038/2231222a0

DO - 10.1038/2231222a0

M3 - Article

AN - SCOPUS:0041426831

SN - 0028-0836

VL - 223

SP - 1222

EP - 1226

JO - Nature

JF - Nature

IS - 5212

ER -

Soft X-Ray background flux

Abstract

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