03693nam a22005415i 4500001001800000003000900018005001700027007001500044008004100059020001800100020001900118024002500137040000900162082001200171100002900183245013000212264004600342300003300388336002600421337002600447338003900473347002400512490006200536505097600598520088301574650001302457650001502470650001802485650002602503650001802529650001302547650004302560650001802603650001502621650004602636650001802682650003002700700002502730700002502755710003402780773002002814776003602834830006202870856009302932942001203025999001703037952009703054978-0-387-26357-1DE-He21320260521091839.0cr nn 008mamaa100301s2005    xxu|    s    |||| 0|eng d  a9780387263571  a997803872635717 a10.1007/b1374472doi  cCICY04a5202231 aKumar, M. S. N.eeditor.10aCores to Clustersh[recurso electrónico] :bA Scientific Autobiography /cedited by M. S. N. Kumar, M. Tafalla, P. Caselli. 1aNew York, NY :bSpringer New York,c2005.  aXV, 222 p.bonline resource.  atextbtxt2rdacontent  acomputerbc2rdamedia  arecurso en líneabcr2rdacarrier  atext filebPDF2rda1 aAstrophysics and Space Science Library,x0067-0057 ;v3240 aReview Articles -- Physical Properties of Prestellar Cores -- Impulsively Triggered Star Formation -- Starless Cores -- Chemical Processes in Star Forming Regions -- Protostellar Jets: A High Angular Resolution Perspective -- Non-Isothermal Gravoturbulent Fragmentation -- The Birth of Massive Stars and Star Clusters -- Precursors of UchII Regions and the Evolution of Massive Outflows -- Observations of Accretion onto High Mass Stars -- Disks Around Massive (proto)Stars -- Embedded Clusters -- Massive Protostars and Small Protoclusters -- Pre-Main-Sequence Evolutionand Brown Dwarfs Beyond the Solar Vicinity -- Brown Dwarfs -- Contributed Poster Articles -- Revealing the Structure of Lupine Darkness: from Cores to Clusters -- Infrared Study of the Southern Galactic Star Forming Region Associated with Iras 10049-5657 -- Studying Protostellar Jets through a Combined Infrared/Optical Spectral Analysis -- Preliminary Results on Newly Discovered Embedded Clusters.  aToward the second half of this decade, several major telescope facilities operating in the infrared, sub-millimeter, and millimeter wave bands will become operational. These missions are expected to throw much light on our understanding of the star formation phenomenon, which is one of the primary science goals in these wave bands. This book contains the proceedings of the "Cores to Clusters" workshop held at Centro de Astrofisica da Universidade do Porto. The mission of the workshop was to discuss current and future issues in star formation physics in the light of these Next Generation Telescopes. This book is comprised of a mixture of articles that provide a comprehensive coverage of current topics including both low and high mass star formation. It serves as a practical compendium for graduate students and young researchers working in the field of star formation. 0aPHYSICS. 0aASTRONOMY. 0aASTROPHYSICS. 0aRELATIVITY (PHYSICS). 0aASTROBIOLOGY.14aPHYSICS.24aASTRONOMY, ASTROPHYSICS AND COSMOLOGY.24aASTROPHYSICS.24aASTRONOMY.24aEXTRATERRESTRIAL PHYSICS, SPACE SCIENCES.24aASTROBIOLOGY.24aRELATIVITY AND COSMOLOGY.1 aTafalla, M.eeditor.1 aCaselli, P.eeditor.2 aSpringerLink (Online service)0 tSpringer eBooks08iPrinted edition:z9780387263229 0aAstrophysics and Space Science Library,x0067-0057 ;v32440uhttp://dx.doi.org/10.1007/b137447zVer el texto completo en las instalaciones del CICY  2ddccER  c32507d32507  00102ddc40708LEaCICYbCICYcELd2025-07-10l0o520r2025-07-10 08:39:36w2025-07-10yER