CO
- Comparative analysis of the far-infrared and (13)CO (J = 0-1) emissions of the Taurus complex
abergel94;
A. Abergel, F. Boulanger, A. Mizuno, Y. Fukui;
ApJ, 1994, 423, L59;
dust, FIR, IRAS, CO, molecular clouds
- Modeling of infrared emission of interstellar clouds - part two - self-consistent models of individual nearby clouds
bernard93;
J. P. Bernard, F. Boulanger, J. L. Puget;
AaA, 1993, 277, 609;
dust, FIR, MIR, IRAS, molecular clouds, CO
- Molecular clouds and galactic spiral structure
cohen80;
R. S. Cohen, H. Cong, T. M. Dame, P. Thaddeus;
ApJ, 1980, 239, L53;
CO, Milky way, H2
- A wide-latitude CO survey of molecular clouds in the northern Milky Way
dame85;
T. M. Dame, P. Thaddeus;
ApJ, 1985, 297, 751;
CO, Milky way, H2
- The largest molecular cloud complexes in the first galactic quadrant
dame86;
T. M. Dame, B. G. Elmegreen, R. S. Cohen, P. Thaddeus;
ApJ, 1986, 305, 892;
CO, Milky way, H2
- A composite CO survey of the entire Milky Way
dame87;
T. M. Dame, H. Ungerechts, R. S. Cohen, E. J. De Geus, I. A. Grenier, J. May, D. C. Murphy, L. A. Nyman, P. Thaddeus;
ApJ, 1987, 322, 706;
CO, Milky way, H2
- The molecular Milky Way
dame88;
T. M. Dame;
ST, 1988, 76, 22;
CO, Milky way, H2
- Molecular Gas at High z in the Milky Way
dame95;
T. M. Dame, P. Thaddeus;
In The Physics of the Interstellar Medium and Intergalactic Medium, 1995, ASP Conference Series, A. Ferrara, C. F. McKee, C. Heiles and P. R. Shapiro, p. 15;
CO, Milky way, H2
- The IRAM key-project: small-scale structure of pre-star-forming regions. I. Observational results
falgarone98;
E. Falgarone, J. F. Panis, A. Heithausen, M. Perault, J. Stutzki, J. L. Puget, F. Bensch;
AaA, 1998, 331, 669;
turbulence, CO, H2, submillimeter
- The structure of the high-latitude molecular cloud toward HD 210121
gredel92;
R. Gredel, E. F. van Dishoeck, C. P. De Vries, J. H. Black;
AaA, 1992, 257, 245;
optical, CO, cirrus, absorption, H2
- Small-area molecular structures without shielding
heithausen2002;
A. Heithausen;
AaA, 2002, 393, L41;
H_I, Ursa Major, CO, cirrus
- Tracing the Molecular Hydrogen Content of the Draco Nebula - Very Low H/H2/W/12CO/ Ratios or Varying Far Infrared Emissivities
herbstmeier93;
U. Herbstmeier, A. Heithausen, U. Mebold;
AaA, 1993, 272, 514;
dust, cirrus, co, H2, h_i, FIR, draco
- A large molecular cloud toward the SNR W50 and SS 433
huang83;
Y. L. Huang, T. M. Dame, P. Thaddeus;
ApJ, 1983, 272, 609;
CO, H2, supershell
- H II regions and CO clouds - The blister model
israel78;
F. P. Israel;
AaA, 1978, 70, 769;
region HII, CO, optical
- Nearby molecular clouds. II - The Cepheus flare and the effect of field stars on galaxy counts
lebrun86;
F. Lebrun;
ApJ, 1986, 306, 16;
CO, H2, supershell
- The Draco nebula - A molecular cloud in the galactic halo?
mebold85;
U. Mebold, J. Cernicharo, L. Velden, K. Reif, C. Crezelius, W. Goerigk;
AaA, 1985, 151, 427;
h_i, h2, cirrus, co, optical, xrays, draco
- Molecular clouds and star formation in the inner galaxy - A comparison of CO, H II, and far-infrared surveys
myers86;
P. C. Myers, T. M. Dame, P. Thaddeus, R. S. Cohen, R. F. Silverberg, E. Dwek, M. G. Hauser;
ApJ, 1986, 301, 398;
CO, FIR, radio continuum, H2, H+, Milky Way, region HII
- Turbulent velocity structure in molecular clouds
ossenkopf2002;
V. Ossenkopf, M. M. Mac Low;
AaA, 2002, 390, 307;
statistical analysis, turbulence, simulation, CO
- Molecular line emission from turbulent clouds
ossenkopf2002a;
V. Ossenkopf;
AaA, 2002, 391, 295;
turbulence, simulation, CO
- The Spectral Correlation Function of Molecular Clouds: A Statistical Test for Theoretical Models
padoan2003;
P. Padoan, A. A. Goodman, M. Juvela;
ApJ, 2003, 588, 881;
statistical analysis, CO, molecular clouds, simulation, turbulence
- Kinematics of the Ursa Major Molecular Clouds
pound97;
M. W. Pound, A. A. Goodman;
ApJ, 1997, 482, 334;
ursa major, CO, H2, cirrus
- Atomic and molecular gas in interstellar cirrus clouds
reach94;
W. T. Reach, B. C. Koo, C. Heiles;
ApJ, 1994, 429, 672;
H_I, H2, CO, 21 cm, dust, FIR, IRAS, draco, cirrus
- Collision of a high-velocity cloud with a dust cloud in the Galactic halo
rohlfs89;
R. Rohlfs, U. Herbstmeier, U. Mebold, A. Winnberg;
AaA, 1989, 211, 402;
H_I, draco, co, cirrus, h2
- Mass, luminosity, and line width relations of Galactic molecular clouds
solomon87;
P. M. Solomon, A. R. Rivolo, J. Barrett, A. Yahil;
ApJ, 1987, 319, 730;
statistical analysis, CO, molecular clouds
- The small scale distribution of interstellar dust from studies of obscured galaxies
thoraval99;
S. Thoraval, P. Boissé, G. Duvert;
AaA, 1999, 351, 1051;
statistical analysis, extinction, molecular clouds, optical, CO
- A molecular cloud forming in the disk-halo interface
weiss99;
A. Weiss, A. Heithausen, U. Herbstmeier, U. Mebold;
AaA, 1999, 344, 955;
cirrus, H_I, CO, 21 cm, H2, FIR, IRAS, dust
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