W43: the closest molecular complex of the Galactic bar?
暂无分享,去创建一个
S. Bontemps | F. Motte | N. Schneider | K. Menten | F. Schuller | T. Henning | P. Schilke | F. Wyrowski | L. Bronfman | Q. N. Luong | F. Heitsch | P. Carlhoff
[1] S. Bontemps,et al. Giving physical significance to the Hi-GAL data: determining the distance of cold dusty cores in the Milky Way , 2011 .
[2] A. Ginsburg,et al. Herschel observations of the W43 “mini-starburst” , 2010, 1005.4092.
[3] J. Ott,et al. MOLECULAR AND ATOMIC GAS IN THE LARGE MAGELLANIC CLOUD. II. THREE-DIMENSIONAL CORRELATION BETWEEN CO AND H i , 2009, 0909.0382.
[4] S. L. Scott,et al. DYNAMICALLY DRIVEN EVOLUTION OF THE INTERSTELLAR MEDIUM IN M51 , 2009, 0907.1656.
[5] J. Rathborne,et al. KINEMATIC DISTANCES TO MOLECULAR CLOUDS IDENTIFIED IN THE GALACTIC RING SURVEY , 2009, 0905.0723.
[6] R. Indebetouw,et al. The Spitzer/GLIMPSE Surveys: A New View of the Milky Way , 2009 .
[7] G. A. Moellenbrock,et al. TRIGONOMETRIC PARALLAXES OF MASSIVE STAR-FORMING REGIONS. VI. GALACTIC STRUCTURE, FUNDAMENTAL PARAMETERS, AND NONCIRCULAR MOTIONS , 2009, 0902.3913.
[8] L. Anderson,et al. RESOLUTION OF THE DISTANCE AMBIGUITY FOR GALACTIC H ii REGIONS , 2008, 0810.5570.
[9] L. Hartmann,et al. Rapid Molecular Cloud and Star Formation: Mechanisms and Movies , 2008, 0808.1078.
[10] N. Rodríguez-Fernández,et al. Gas flow models in the Milky Way embedded bars , 2008, 0806.4252.
[11] P. Goldsmith,et al. Resolving distance ambiguities towards 6.7 GHz methanol masers , 2008, 0805.2697.
[12] R. Klessen,et al. From the warm magnetized atomic medium to molecular clouds , 2008, 0805.1366.
[13] S. Bontemps,et al. The earliest phases of high-mass star formation: a 3 square degree millimeter continuum mapping of Cygnus X , 2007, 0708.2774.
[14] E. Bergin,et al. Dust and gas emission in the prototypical hot core G29.96-0.02 at sub-arcsecond resolution , 2007, 0704.0518.
[15] R. Klessen,et al. Molecular Cloud Evolution. II. From Cloud Formation to the Early Stages of Star Formation in Decaying Conditions , 2006, astro-ph/0608375.
[16] T. Mahoney,et al. The Long Bar in the Milky Way: Corroboration of an Old Hypothesis , 2006, astro-ph/0606201.
[17] J. Stil,et al. Accepted for Publication in the Astronomical Journal the Vla Galactic Plane Survey Accepted for Publication in the Astronomical Journal , 2022 .
[18] J. Rathborne,et al. The Boston University-Five College Radio Astronomy Observatory Galactic Ring Survey , 2005, astro-ph/0602160.
[19] Chen Cao,et al. PAH and Mid-Infrared Luminosities as Measures of Star Formation Rate in Spitzer First Look Survey Galaxies , 2005, astro-ph/0509281.
[20] L. Chomiuk,et al. First GLIMPSE Results on the Stellar Structure of the Galaxy , 2005, astro-ph/0508325.
[21] E. Peeters,et al. Polycyclic Aromatic Hydrocarbons as a Tracer of Star Formation? , 2004 .
[22] R. Indebetouw,et al. GLIMPSE. I. An SIRTF Legacy Project to Map the Inner Galaxy , 2003, astro-ph/0306274.
[23] F. Motte,et al. From Massive Protostars to a Giant H II Region: Submillimeter Imaging of the Galactic Ministarburst W43 , 2002, astro-ph/0208519.
[24] D. Russeil,et al. Star-forming complexes and the spiral structure of our Galaxy , 2003 .
[25] Jean-Luc Starck,et al. Astronomical image and data analysis , 2002 .
[26] T. M. Bania,et al. The Structure of Four Molecular Cloud Complexes in the BU-FCRAO Milky Way Galactic Ring Survey , 2001 .
[27] J. Carpenter,et al. The Equilibrium State of Molecular Regions in the Outer Galaxy , 2001, astro-ph/0101133.
[28] D. Hartmann,et al. The Milky Way in Molecular Clouds: A New Complete CO Survey , 2000, astro-ph/0009217.
[29] P. Kroupa. On the variation of the initial mass function , 2000, astro-ph/0009005.
[30] T. Mahoney,et al. Detection of the old stellar component of the major Galactic bar , 2000, astro-ph/0007232.
[31] E. Bergin,et al. High-Angular Resolution Millimeter-Wave and Near-Infrared Imaging of the Ultracompact H II Region G29.96–0.02 , 1999 .
[32] P. Conti,et al. The Stellar Content of Obscured Galactic Giant H II Regions. II. W42 , 1998, astro-ph/0001157.
[33] J. Carpenter,et al. The W51 Giant Molecular Cloud , 1998, astro-ph/9806298.
[34] Jr.,et al. The Global Schmidt law in star forming galaxies , 1997, astro-ph/9712213.
[35] A. Watson,et al. Near-Infrared Spectroscopy of G29.96–0.02: The First Spectral Classification of the Ionizing Star of an Ultracompact H II Region , 1997, astro-ph/9709120.
[36] J. Silk. Feedback, Disk Self-Regulation, and Galaxy Formation , 1996, astro-ph/9612117.
[37] H. Liszt. Molecular Gas in the Core of W43 (G30.8+0.0) , 1995 .
[38] L. Blitz,et al. Proto--Brown Dwarfs. I. Methods and Results for High-Latitude Clouds , 1993 .
[39] R. Rand. Density wave kinematics and giant molecular association formation in M51 , 1993 .
[40] R. Rand,et al. M51: molecular spiral arms, giant molecular associations, and superclouds , 1990 .
[41] E. Churchwell,et al. Massive stars embedded in molecular clouds - Their population and distribution in the galaxy , 1989 .
[42] B. Elmegreen,et al. H I superclouds in the inner Galaxy , 1987 .
[43] A. R. Rivolo,et al. Mass, luminosity, and line width relations of Galactic molecular clouds , 1987 .
[44] B. Elmegreen,et al. The largest molecular cloud complexes in the first galactic quadrant , 1986 .
[45] T. L. Wilson,et al. Tools of Radio Astronomy , 1986 .
[46] R. L. Brown,et al. Star formation in the inner Galaxy - A far-infrared and radio study of two H II regions , 1985 .
[47] Lyman Spitzer,et al. Physical processes in the interstellar medium , 1998 .