NAME Eridanus Cavity , the SIMBAD biblio

NAME Eridanus Cavity , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:50:52

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1988A&A...196..255V 69 T                   1 43 6 Search for an excess rotation measure in the shell around the Eridanus cavity. VALLEE J.P., MacLEOD J.M. and BROTEN N.W.
2007ApJ...658.1081G 2 7 47 XMM-Newton observations of the diffuse X-ray background. GALEAZZI M., GUPTA A., COVEY K., et al.
2009ApJ...695.1127G 503       D     X C F     12 10 21 Evidence for the missing baryons in the angular correlation of the diffuse X-ray background. GALEAZZI M., GUPTA A. and URSINO E.
2009ApJ...702..270G 127       D     X         4 8 7 Contribution of unresolved point sources to the diffuse X-ray background below 1 keV. GUPTA A. and GALEAZZI M.
2009ApJ...707..644G 1591       D S   X C F     40 4 27 Properties of the diffuse X-ray background toward MBM20 with Suzaku. GUPTA A., GALEAZZI M., KOUTROUMPA D., et al.
2010A&A...520A..51V 173     A     X         5 33 24 Probing the evolving massive star population in Orion with kinematic and radioactive tracers. VOSS R., DIEHL R., VINK J.S., et al.
2012ApJ...755..166H 39           X         1 10 27 The ElIXr galaxy survey. II. Baryons and dark matter in an isolated elliptical galaxy. HUMPHREY P.J., BUOTE D.A., O'SULLIVAN E., et al.
2014A&A...566A..94K 139     A     X         4 15 16 Feedback by massive stars and the emergence of superbubbles. II. X-ray properties. KRAUSE M., DIEHL R., BOEHRINGER H., et al.
2019A&A...625A.135L viz 64           X         1 10 231 Gaia-2MASS 3D maps of Galactic interstellar dust within 3 kpc. LALLEMENT R., BABUSIAUX C., VERGELY J.L., et al.
2022PASJ...74.1396U 17       D               1 89 2 The soft X-ray background with Suzaku. I. Milky Way halo. UEDA M., SUGIYAMA H., KOBAYASHI S.B., et al.
2023ApJ...947...49H 87             C       1 5 ~ Point-source Contribution to the Diffuse X-Ray Background below 1 keV and Its Effect on Our Understanding of the Circumgalactic Medium. HUANG S., CAPPELLUTI N., GALEAZZI M., et al.
2025ApJ...989..194G 47           X         1 13 ~ Where Is the Supervirial Gas? III. Insights from X-Ray Shadow Observations and a Revised Model for the Soft Diffuse X-Ray Background. GUPTA A., MATHUR S., KINGSBURY J., et al.

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