NAME Ori-Eri , the SIMBAD biblio

NAME Ori-Eri , the SIMBAD biblio (26 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST17:37:11


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Title First 3 Authors
1988A&AS...74...63M 25 6 Linear polarizations in selected celestial zones. The Orion-Eridanus area. MacLEOD J.M., VALLEE J.P. and BROTEN N.W.
1988ApJ...333..341R 28 75 S II / H-alpha intensity ratios in faint, extended HII regions and the origin of the interstellar emission-line background. REYNOLDS R.J.
1995ApJ...439..399S 18 33 ROSAT observations of the Eridanus soft X-ray enhancement. SNOWDEN S.L., BURROWS D.N., SANDERS W.T., et al.
1997FCPh...18....1P 2 12 117 The Gould Belt system and the local interstellar medium. POEPPEL W.
1999ApJS..124..465W 14 4 168 The diffuse interstellar clouds toward 23 Orionis. WELTY D.E., HOBBS L.M., LAUROESCH J.T., et al.
2000PASP..112.1542M 8 3 Modified Stromgren sphere. McCULLOUGH P.R.
2004NewAR..48..763V 144 144 Cosmic magnetic fields - as observed in the Universe, in galactic dynamos, and in the Milky Way. VALLEE J.P.
2005A&A...430..523W 1 27 137 A uniform CO survey of the molecular clouds in Orion and Monoceros. WILSON B.A., DAME T.M., MASHEDER M.R.W., et al.
2005MNRAS.364.1185P 1 6 32 Cosmic microwave background and foregrounds in Wilkinson Microwave Anisotropy Probe first-year data. PATANCHON G., CARDOSO J.-F., DELABROUILLE J., et al.
2009Ap.....52..168G 37           X         1 40 0 Star formation and molecular clouds. GYULBUDAGHIAN A.L.
2011NewAR..55...91V 38           X         1 218 40 Magnetic fields in the galactic Universe, as observed in supershells, galaxies, intergalactic and cosmic realms. VALLEE J.P.
2013ApJ...770...78C 41           X         1 11 84 The structure, origin, and evolution of interstellar hydrocarbon grains. CHIAR J.E., TIELENS A.G.G.M., ADAMSON A.J., et al.
2014A&A...566A..94K         O           15 16 Feedback by massive stars and the emergence of superbubbles. II. X-ray properties. KRAUSE M., DIEHL R., BOEHRINGER H., et al.
2015ApJ...801..142B 172       D     X C       4 15 13 The galactic 26Al emission map as revealed by INTEGRAL SPI. BOUCHET L., JOURDAIN E. and ROQUES J.-P.
2015ApJ...808..111O 530     A     X         14 44 29 Nested shells reveal the rejuvenation of the Orion-Eridanus superbubble. OCHSENDORF B.B., BROWN A.G.A., BALLY J., et al.
2016AJ....151..147S 79           X         2 12 2 The ionization structure of Sharpless 2-264: multiwavelength observations of the λ Ori H II region. SAHAN M. and HAFFNER L.M.
2017MNRAS.468.2957R 294       D     X C F     6 15 7 A new perspective on turbulent Galactic magnetic fields through comparison of linear polarization decomposition techniques. ROBITAILLE J.-F., SCAIFE A.M.M., CARRETTI E., et al.
2018ApJ...866...34S 361           X C       8 13 ~ Ultraviolet line intensities of intermediate and high ions predicted from non-equilibrium ionization simulations. SHELTON R.L. and KWAK K.
2020A&A...639A.110A 1301     A S   X C       30 41 ~ Large-scale [C II] 158 µm emission from the Orion-Eridanus superbubble. ABDULLAH A. and TIELENS A.G.G.M.
2021ApJ...919L...5B 47           X         1 6 31 The Per-Tau Shell: a giant star-forming spherical shell revealed by 3D dust observations. BIALY S., ZUCKER C., GOODMAN A., et al.
2022A&A...658A..98P 43           X         1 47 4 [C II] 158 µm line emission from Orion A. II. Photodissociation region physics. PABST C.H.M., GOICOECHEA J.R., HACAR A., et al.
2022MNRAS.513.5900H 170           X   F     3 13 10 The C-Band All-Sky Survey (C-BASS): template fitting of diffuse galactic microwave emission in the northern sky. HARPER S.E., DICKINSON C., BARR A., et al.
2022ApJ...940...75D 43           X         1 11 6 Structure in the Magnetic Field of the Milky Way Disk and Halo Traced by Faraday Rotation. DICKEY J.M., WEST J., THOMSON A.J.M., et al.
2023ApJ...947...66F 87           X         2 34 3 A 3D View of Orion. I. Barnard's Loop. FOLEY M.M., GOODMAN A., ZUCKER C., et al.
2024A&A...685A.102K 90             C       1 8 ~ Cosmic-ray diffusion in two local filamentary clouds. KAMAL YOUSSEF F.R. and GRENIER I.A.
2025A&A...702A.220Y 47           X         1 27 ~ Imaging the positron annihilation line with 20 years of INTEGRAL/SPI observations. YONEDA H., SIEGERT T. and MITTAL S.

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