L1599B: CLOUD ENVELOPE AND C+ EMISSION IN A REGION OF MODERATELY ENHANCED RADIATION FIELD
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[1] M. Juvela,et al. PLANCK COLD CLUMPS IN THE λ ORIONIS COMPLEX. I. DISCOVERY OF AN EXTREMELY YOUNG CLASS 0 PROTOSTELLAR OBJECT AND A PROTO-BROWN DWARF CANDIDATE IN THE BRIGHT-RIMMED CLUMP PGCC G192.32–11.88 , 2015, 1511.09121.
[2] P. Goldsmith,et al. HERSCHEL GALACTIC PLANE SURVEY OF [N ii] FINE STRUCTURE EMISSION , 2015, 1510.05706.
[3] H. Müller,et al. VELOCITY-RESOLVED [C ii] EMISSION AND [C ii]/FIR MAPPING ALONG ORION WITH HERSCHEL , 2015, The Astrophysical journal.
[4] P. Goldsmith,et al. PHOTON-DOMINATED REGION MODELING OF THE [C i], [C ii], AND CO LINE EMISSION FROM A BOUNDARY IN THE TAURUS MOLECULAR CLOUD , 2014, 1409.1210.
[5] Y. Sekimoto,et al. FLASH$^{+}$ —A Dual-Channel Wide-Band Spectrometer for APEX , 2014, IEEE Transactions on Terahertz Science and Technology.
[6] H. Rix,et al. A LARGE CATALOG OF ACCURATE DISTANCES TO MOLECULAR CLOUDS FROM PS1 PHOTOMETRY , 2014, 1403.3393.
[7] P. Goldsmith,et al. C+ IN THE INTERSTELLAR MEDIUM: COLLISIONAL EXCITATION BY H2 REVISITED , 2013, 1312.0282.
[8] P. Goldsmith. DIFFUSE MOLECULAR CLOUD DENSITIES FROM UV MEASUREMENTS OF CO ABSORPTION , 2013, 1307.8374.
[9] P. Goldsmith,et al. A Herschel [C ii] Galactic plane survey - I. The global distribution of ISM gas components , 2013, 1304.7770.
[10] J. Greenberg,et al. Interstellar Dust and Related Topics , 2012 .
[11] Sheng Li,et al. Development of Superconducting Spectroscopic Array Receiver: A Multibeam 2SB SIS Receiver for Millimeter-Wave Radio Astronomy , 2012, IEEE Transactions on Terahertz Science and Technology.
[12] P. Goldsmith,et al. COLLISIONAL EXCITATION OF THE [C ii] FINE STRUCTURE TRANSITION IN INTERSTELLAR CLOUDS , 2012, 1209.4536.
[13] Erin C. Smith,et al. EARLY SCIENCE WITH SOFIA, THE STRATOSPHERIC OBSERVATORY FOR INFRARED ASTRONOMY , 2012, 1205.0791.
[14] Andreas Bell,et al. GREAT : early science results Special feature L etter to the E ditor High-resolution wide-band fast Fourier transform spectrometers , 2012 .
[15] U. U. Graf,et al. GREAT: the SOFIA high-frequency heterodyne instrument , 2012, 1203.2845.
[16] Y. Okada,et al. GREAT/SOFIA atmospheric calibration , 2012, 1203.1661.
[17] M. Lombardi,et al. 2MASS wide field extinction maps - IV. The Orion, Monoceros R2, Rosette, and Canis Major star forming regions , 2011, 1107.5096.
[18] D. Byun,et al. 100-GHZ BAND TEST OBSERVATIONS OF THE KVN 21-M RADIO TELESCOPES , 2011 .
[19] J. Peek,et al. THE GALFA-Hi SURVEY: DATA RELEASE 1 , 2011, 1101.1879.
[20] Di Li,et al. THE RELATION BETWEEN GAS AND DUST IN THE TAURUS MOLECULAR CLOUD , 2010, 1007.5060.
[21] S. Ott,et al. Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy , 2010, 1005.5331.
[22] D. Padgett,et al. EVIDENCE FOR DUST EVOLUTION WITHIN THE TAURUS COMPLEX FROM SPITZER IMAGES , 2009, 0906.5025.
[23] Michael Olberg,et al. A Swedish heterodyne facility instrument for the APEX telescope , 2008 .
[24] H. Liszt. Formation, fractionation and excitation of carbon monoxide in diffuse clouds , 2007, 0710.2237.
[25] J. Black,et al. A computer program for fast non-LTE analysis of interstellar line spectra With diagnostic plots to interpret observed line intensity ratios , 2007, 0704.0155.
[26] Catherine J. Cesarsky,et al. The Atacama Pathfinder EXperiment (APEX) : a new submillimeter facility for southern skies , 2006 .
[27] J. L. Bourlot,et al. A Model for Atomic and Molecular Interstellar Gas: The Meudon PDR Code , 2006, astro-ph/0602150.
[28] C. Kramer,et al. The Herschel-Heterodyne Instrument for the Far-Infrared (HIFI) , 2005, Infrared and Millimeter Waves, Conference Digest of the 2004 Joint 29th International Conference on 2004 and 12th International Conference on Terahertz Electronics, 2004..
[29] A. Tielens,et al. Neutral Atomic Phases of the Interstellar Medium in the Galaxy , 2003 .
[30] D. Hollenbach,et al. Time Dependence of the Ultraviolet Radiation Field in the Local Interstellar Medium , 2002, astro-ph/0202196.
[31] Di Li,et al. H I Narrow Self-Absorption in Dark Clouds: Correlations with Molecular Gas and Implications for Cloud Evolution and Star Formation , 2002, astro-ph/0206396.
[32] M. Lombardi,et al. Mapping the interstellar dust with near-infrared observations: An optimized multi-band technique , 2001, astro-ph/0109135.
[33] R. Mathieu,et al. The Spatial Distribution of the λ Orionis Pre-Main-Sequence Population , 2001 .
[34] Alexander G. G. M. Tielens,et al. Photodissociation Regions in the Interstellar Medium of Galaxies , 1999 .
[35] M. Masheder,et al. CO Observations of the λ-Orionis Ring , 1998, Publications of the Astronomical Society of Australia.
[36] A. Penzias,et al. (C-12)/(C-13) isotope ratio in the local interstellar medium from observations of (C-13)(O-18) in molecular clouds , 1993 .
[37] B. Andersson,et al. Warm neutral halos around molecular clouds. VI - Physical and chemical modeling , 1993 .
[38] I. Gatley,et al. A spectroscopic study of the Dr 21 outflow source. III - The CO line emission , 1991 .
[39] M. Morris,et al. An Expanding System of Molecular Clouds Surrounding lambda Orionis , 1987 .
[40] P. Goldsmith,et al. A detailed examination of the kinematics of rotating dark clouds , 1986 .
[41] S. Lichten,et al. Warm H I Halos around molecular clouds , 1983 .
[42] C. Lada,et al. Star formation in the lambda orionis region. I. The distribution of young objects , 1982 .
[43] P. Murdin,et al. The Lambda Orionis association , 1977 .
[44] R. Balian,et al. Atomic and molecular physics and interstellar matter , 1975 .
[45] C. M. Wade. A 21-cm line study of an expanding HIl region. , 1957 .