Fermi-LATγ-Ray Study of the Interstellar Medium and Cosmic Rays in the Chamaeleon Molecular Cloud Complex: A Look at the Dark Gas as Optically Thick H i
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Yasuo Fukui | Tsunefumi Mizuno | Hiroaki Yamamoto | Naoya Hidaka | Hiroyasu Tajima | Hidetoshi Sano | Akira Okumura | Katsuhiro Hayashi | Ryuji Okamoto
[1] Igor V. Moskalenko,et al. Cosmic-Ray Propagation and Interactions in the Galaxy , 2007 .
[2] P. Andre',et al. CHANGES OF DUST OPACITY WITH DENSITY IN THE ORION A MOLECULAR CLOUD , 2012, 1211.6475.
[3] G. W. Pratt,et al. Planck intermediate results. XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies , 2013, 1312.5446.
[4] The Fermi-LAT Collaboration. Fermi Large Area Telescope Third Source Catalog , 2015, 1501.02003.
[5] D. Schlegel,et al. Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds , 1997, astro-ph/9710327.
[6] J. Chiang,et al. ERRATUM: “FERMI LARGE AREA TELESCOPE STUDY OF COSMIC-RAYS AND THE INTERSTELLAR MEDIUM IN NEARBY MOLECULAR CLOUDS” (2012, ApJ, 755, 22) , 2013 .
[7] T. Hayakawa,et al. A New Derivation of the Extinction-to-CO Column Density Ratio in the Chamaeleon I Dark Cloud , 1999 .
[8] C. A. Oxborrow,et al. Planck 2013 results. XIII. Galactic CO emission , 2013, 1303.5073.
[9] H. Yamamoto,et al. OPTICALLY THICK H i DOMINANT IN THE LOCAL INTERSTELLAR MEDIUM: AN ALTERNATIVE INTERPRETATION TO “DARK GAS” , 2014, 1403.0999.
[10] P. Kalberla,et al. GASS: The Parkes Galactic All-Sky Survey - Update: improved correction for instrumental effects and new data release , 2015, 1505.01011.
[11] H. Yamamoto,et al. QUANTIFYING THE INTERSTELLAR MEDIUM AND COSMIC RAYS IN THE MBM 53, 54, AND 55 MOLECULAR CLOUDS AND THE PEGASUS LOOP USING FERMI-LAT GAMMA-RAY OBSERVATIONS , 2016, 1610.08596.
[12] J. Casandjian. LOCAL H i EMISSIVITY MEASURED WITH FERMI-LAT AND IMPLICATIONS FOR COSMIC-RAY SPECTRA , 2015 .
[13] G. W. Pratt,et al. Planck 2015 results - X. Diffuse component separation: Foreground maps , 2015, 1502.01588.
[14] A. Strong,et al. Propagation of Cosmic-Ray Nucleons in the Galaxy , 1998, astro-ph/9807150.
[15] J. Chiang,et al. THE LARGE AREA TELESCOPE ON THE FERMI GAMMA-RAY SPACE TELESCOPE MISSION , 2009, 0902.1089.
[16] Y. Fukui,et al. A Large Scale 12CO (J=1−0) Survey toward the Chamaeleon Region with NANTEN , 2001 .
[17] Vlasios Vasileiou,et al. THE FERMI LARGE AREA TELESCOPE ON ORBIT: EVENT CLASSIFICATION, INSTRUMENT RESPONSE FUNCTIONS, AND CALIBRATION , 2012 .
[18] B. Savage,et al. A survey of interstellar H I from L-alpha absorption measurements. II , 1978 .
[19] S. Digel,et al. EGRET Observations of the Diffuse Gamma-Ray Emission in Orion: Analysis through Cycle 6 , 1999, astro-ph/9902214.
[20] K. Hayashi,et al. H i, CO, and Dust in the Perseus Cloud , 2016, 1612.07696.
[21] D. L. Bertsch,et al. The Likelihood Analysis of EGRET Data , 1996 .
[22] M. Halpern,et al. EVIDENCE FOR ENVIRONMENTAL CHANGES IN THE SUBMILLIMETER DUST OPACITY , 2011, 1112.5433.
[23] T. Brandt,et al. A Method for Exploring Systematics Due to Galactic Interstellar Emission Modeling: Application to the Fermi LAT SNR Catalog , 2013, 1304.1395.
[24] R. Klessen,et al. Modelling CO emission – I. CO as a column density tracer and the X factor in molecular clouds , 2010, 1011.2019.
[25] D. Schlegel,et al. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .
[26] D. Thompson,et al. FERMI LARGE AREA TELESCOPE STUDY OF COSMIC RAYS AND THE INTERSTELLAR MEDIUM IN NEARBY MOLECULAR CLOUDS , 2012 .
[27] J. Chiang,et al. GAMMA-RAY OBSERVATIONS OF THE ORION MOLECULAR CLOUDS WITH THE FERMI LARGE AREA TELESCOPE , 2012, The Astrophysical Journal.
[28] K. Hayashi,et al. Synthetic Observations of 21 cm H i Line Profiles from Inhomogeneous Turbulent Interstellar H i Gas with Magnetic Fields , 2017, The Astrophysical Journal.
[29] C. A. Oxborrow,et al. Planck intermediate results - XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck , 2014, 1409.3268.
[30] J. Dickey,et al. , CO, AND PLANCK/IRAS DUST PROPERTIES IN THE HIGH LATITUDE CLOUD COMPLEX, MBM 53, 54, 55 AND HLCG 92 − 35. POSSIBLE EVIDENCE FOR AN OPTICALLY THICK ENVELOPE AROUND THE CO CLOUDS , 2014, 1401.7398.
[31] J. Peek,et al. Optically Thick H i Does Not Dominate Dark Gas in the Local ISM , 2018, The Astrophysical Journal.
[32] M. Mori. Nuclear enhancement factor in calculation of Galactic diffuse gamma-rays: A new estimate with DPMJET-3 , 2009, 0903.3260.
[33] M. Pérault,et al. Diffuse infrared emission from the galaxy. I: Solar neighborhood , 1988 .
[34] S. Digel,et al. Gamma-ray observations of Ophiuchus with EGRET: The diffuse emission and point sources , 1994 .
[35] B. Reipurth. Handbook of Star Forming Regions, Volume I: The Northern Sky , 2008 .
[36] A. Franckowiak,et al. FERMI-LAT OBSERVATIONS OF HIGH- AND INTERMEDIATE-VELOCITY CLOUDS: TRACING COSMIC RAYS IN THE HALO OF THE MILKY WAY , 2015, The Astrophysical journal.
[37] K. Gorski,et al. HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere , 2004, astro-ph/0409513.
[38] A. Strong,et al. Inverse Compton Origin of the Hard X-Ray and Soft Gamma-Ray Emission from the Galactic Ridge , 2008, 0804.1774.
[39] C. Dominik,et al. UvA-DARE ( Digital Academic Repository ) Dust coagulation and fragmentation in molecular clouds : II . The opacity of the dust aggregate size distribution , 2011 .
[40] D. Thompson,et al. CONSTRAINTS ON THE COSMIC-RAY DENSITY GRADIENT BEYOND THE SOLAR CIRCLE FROM FERMI γ-RAY OBSERVATIONS OF THE THIRD GALACTIC QUADRANT , 2010, 1011.0816.
[41] D. Marshall,et al. Cosmic rays, gas and dust in nearby anticentre clouds : I -- CO-to-H2 conversion factors and dust opacities , 2017, 1703.05237.
[42] C. Heiles,et al. THE MILLENNIUM ARECIBO 21-CM ABSORPTION LINE SURVEY . II . PROPERTIES OF THE WARM AND COLD NEUTRAL MEDIA , 2002 .
[43] C. B. Netterfield,et al. Planck early results. XIX. All-sky temperature and dust optical depth from Planck and IRAS. Constraints on the "dark gas" in our Galaxy , 2011, 1101.2029.
[44] R. Klessen,et al. CO-dark gas and molecular filaments in Milky Way-type galaxies , 2014, 1403.1589.
[45] G. W. Pratt,et al. Planck 2013 results. XI. All-sky model of thermal dust emission , 2013, 1312.1300.
[46] T. Dame,et al. Molecular Clouds in the Milky Way , 2015 .
[47] A. Cox,et al. Allen's astrophysical quantities , 2000 .
[48] T. Hayakawa,et al. CO Column Density and Extinction in the Chamaeleon II--III Dark-Cloud Complex , 2001 .
[49] Christopher F. McKee,et al. THE DARK MOLECULAR GAS , 2010, 1004.5401.
[50] S. Inutsuka,et al. FORMATION OF TURBULENT AND MAGNETIZED MOLECULAR CLOUDS VIA ACCRETION FLOWS OF H i CLOUDS , 2012, 1205.6217.
[51] D. Marshall,et al. Cosmic-rays, gas, and dust in nearby anticentre clouds : II -- Interstellar phase transitions and the Dark Neutral Medium , 2017, 1711.05506.
[52] D. Bhattacharya,et al. A New Σ-D Relation and Its Application to the Galactic Supernova Remnant Distribution , 1998, astro-ph/9807162.
[53] Isabelle A. Grenier,et al. Unveiling Extensive Clouds of Dark Gas in the Solar Neighborhood , 2005, Science.
[54] J. Dickey,et al. H I in the Galaxy , 1990 .