W 3h , the SIMBAD biblio

W 3h , the SIMBAD biblio (27 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST05:51:39


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Title First 3 Authors
1973A&A....29..369S 14 48 Line and continuum synthesis of W 3. SULLIVAN III W.T. and DOWNES D.
1980MNRAS.193..495C 15 55 Radio observations of W3 at 2.7 and 14.4GHz. COLLEY D.
1983A&A...125..320D 12 19 A comparison of high resolution optical and radio observations of W3. DICKEL H.R., HARTEN R.H. and GULL T.R.
1990A&A...238..296V 11 16 High resolution HI observations of HII regions. II. HI and the magnetic field near W 3. VAN DER WERF P.P. and GOSS W.M.
1995A&A...303..901T 15 27 The W 3 core: masses, densities, sizes and kinematics. TIEFTRUNK A.R., WILSON T.L., STEPPE H., et al.
1996ApJ...471..871A 11 13 Helium enrichment and carbon ionization in the W3 core. ADLER D.S., WOOD D.O.S. and GOSS W.M.
1997A&A...318..931T 35 68 The H II/molecular cloud complex W3 revisited: imaging the radio continuum sources using multi-configuration, multi-frequency observations with the VLA. TIEFTRUNK A.R., GAUME R.A., CLAUSSEN M.J., et al.
1998A&A...340..232T 17 19 High-resolution imaging of NH3 inversion lines toward W3 main. TIEFTRUNK A.R., GAUME R.A. and WILSON T.L.
1998AJ....116.1323K 47 123 Shock-excited maser emission from supernova remnants: G32.8-0.1, G337.8-0.1, G346.6-0.2, and the HB 3/W3 complex. KORALESKY B., FRAIL D.A., GOSS W.M., et al.
1998ApJ...504..375K 14 19 VLA observations of hydrogen and carbon recombination lines toward W3A at 1.4 GHz. KANTHARIA N.G., ANANTHARAMAIAH K.R. and GOSS W.M.
1999AJ....117.2440N 24 13 Probing the interstellar medium using H I absorption and emission toward the W3 H II region. NORMANDEAU M.
1999PASP..111.1049G 128 313 Massive stars: their environment and formation. (Invited review). GARAY G. and LIZANO S.
2000ApJ...535..913S 26 29 Probing the magnetic field structure in the W3 molecular cloud. SCHLEUNING D.A., VAILLANCOURT J.E., HILDEBRAND R.H., et al.
2002ApJ...579L..95H 22 33 X-ray detection of the ionizing stars in ultracompact H II regions. HOFNER P., DELGADO H., WHITNEY B., et al.
2004A&A...424..887K 34 43 Emission of CO, CI, and CII in W3Main. KRAMER C., JAKOB H., MOOKERJEA B., et al.
2004ApJ...608..797O 31 51 Deep near-infrared observations of the W3 main star-forming region. OJHA D.K., TAMURA M., NAKAJIMA Y., et al.
2006BASI...34..119O 14 5 Luminosity functions of YSO clusters in Sh-2 255, W 3 main and NGC 7538 star forming regions. OJHA D., TAMURA M. (The Sirius Team)
2007ApJ...654..338R viz 20 20 Spitzer observations of the giant molecular cloud W3. RUCH G.T., JONES T.J., WOODWARD C.E., et al.
2008ApJ...673..354F 38           X         1 37 61 The diverse stellar populations of the W3 star-forming complex. FEIGELSON E.D. and TOWNSLEY L.K.
2011MNRAS.411..705M viz 38           X         1 105 43 Spectrophotometric distances to Galactic H II regions. MOISES A.P., DAMINELI A., FIGUEREDO E., et al.
2012ApJ...744...87B 132       D     X         4 39 45 Age spread in W3 Main: large binocular Telescope/LUCI near-infrared spectroscopy of the massive stellar content. BIK A., HENNING Th., STOLTE A., et al.
2012ApJ...749L..21S 39           X         1 13 17 First science results from SOFIA/FORCAST: the mid-infrared view of the compact H II region W3A. SALGADO F., BERNE O., ADAMS J.D., et al.
2012ApJ...754...87W 155           X         4 31 12 Different evolutionary stages in the massive star-forming region W3 main complex. WANG Y., BEUTHER H., ZHANG Q., et al.
2014A&A...561A..12B viz 118           X C       2 36 16 Deep near-infrared imaging of W3 Main: constraints on stellar cluster formation. BIK A., STOLTE A., GENNARO M., et al.
2020A&A...636A.118M 43           X         1 26 ~ From clump to disc scales in W3 IRS4. A case study of the IRAM NOEMA large programme CORE. MOTTRAM J.C., BEUTHER H., AHMADI A., et al.
2021ApJ...917...47R 174           X         4 17 4 Shocked molecular hydrogen and broad CO lines from the interacting supernova remnant HB 3. RHO J., JARRETT T.H., TRAM L.N., et al.
2023ApJ...952..102G 187           X C       3 13 ~ Structure of the W3A Low-density Foreground Region. GOLDSMITH P.F., LANGER W.D., SEO Y., et al.

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