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The Role of Dust in the Formation of Stars

Proceedings of the ESO Workshop Held at Garching, Germany, 11–14 September 1995

  • Conference proceedings
  • © 1996

Overview

Editors:
  1. Hans Ulrich Käufl

    1. European Southern Observatory, Garching, Germany

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  2. Ralf Siebenmorgen

    1. Villafranca del Castillo, Satellite Tracking Station, ESA, Madrid, Spain

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    You can also search for this editor in PubMed   Google Scholar

Part of the book series: ESO Astrophysics Symposia (ESO)

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Table of contents (92 papers)

  1. Front Matter

    Pages I-XXII
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  2. Ground-Based Observations of Young Stellar Objects

    1. Front Matter

      Pages 1-1
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    2. High-Angular Resolution Near-Infrared Observations of the Circumstellar Environment of Young Stellar Objects

      • N. Ageorges, A. Eckart
      Pages 3-6

    3. Submillimeter Dust Continuum Emission as a Probe of Protostellar Evolution

      • Philippe André, Sylvain Bontemps
      Pages 7-10

    4. Compact Molecular Outflows from Young Stellar Objects in L1641

      • J. C. Correia, M. Griffin, P. Saraceno, A. Zavagno
      Pages 11-14

    5. Anatomy of a Spatially Resolved Dust Disc Around a B-Type YSO

      • W. R. F. Dent, C. Racela, F. Rosengarten
      Pages 15-18

    6. Mid-IR PAH Emission in YSOs WL 16 & WL 22

      • J. P. Emerson
      Pages 19-22

    7. Mid-IR Imaging of YSOs: the Hydrocarbon Emission Features in WL 16

      • J. P. Emerson, T. J. T. Moore, C. J. Skinner, M. M. Meixner
      Pages 23-26

    8. Star Formation in the Vela Molecular Clouds: Near IR Images

      • T. Giannini, D. Lorenzetti, B. Nisini, L. Spinoglio, A. Zavagno, R. Liseau et al.
      Pages 27-30

    9. Linear and Circular Imaging Polarimetry of the Chamaeleon Infrared Nebula

      • T. M. Gledhill, A. Chrysostomou, J. H. Hough
      Pages 31-34

    10. Near-IR Speckle Imaging of Luminous Young Stellar Objects

      • Melvin G. Hoare, Andreas Glindemann, Andrea Richichi
      Pages 35-38

    11. A Large Dust Shell Observed at 10µm Around V921 Sco

      • Pierre-Olivier Lagage, Sylvie Cabrit, Thierry Montmerle, Göran Olofsson
      Pages 39-42

    12. Dust Emission from Bok Globules

      • Ralf Launhardt, Thomas Henning
      Pages 43-46

    13. Density Structure of Protostellar Envelopes

      • F. Motte, P. André, R. Neri
      Pages 47-50

    14. What Causes the Variability of the PV Cep Nebula?

      • Th. Neckel, H. J. Staude
      Pages 51-54

    15. 1.3 mm Dust Continuum Observations of Young X-ray Selected Stars in Ophiuchus

      • Dieter Nürnberger, Wolfgang Brandner, Harold W. Yorke, Hans Zinnecker
      Pages 55-58

    16. The Luminosity-mm Flux Correlation of Class I Sources Exciting Outflows

      • P. Saraceno, F. D’Antona, F. Palla, M. Griffin, E. Tommasi
      Pages 59-62

    17. PAHs as Probes of Photo-Dissociation Regions in M17 and the Orion Bar

      • G. C. Sloan, J. Bregman, A. S. B. Schultz, P. Temi, D. M. Rank
      Pages 63-66

    18. Mid-Infrared Imaging Polarimetry of BNKL

      • Craig H. Smith, David K. Aitken, Toby J. T. Moore, Takuya Fujiyoshi, Patrick F. Roche, Christopher M. Wright
      Pages 67-70

    19. Star Formation in the Northern Region of NGC 6334

      • Mauricio Tapia, Paolo Persi
      Pages 71-74
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Keywords

About this book

This ESO workshop, which took place in September 1995 on a topic that at a first glance could be considered rather specialized, attracted an unpre­ dictably large number of scientists. This certainly reflects the importance of this field, which has lost its seemingly esoteric character, in a wider astro­ physical context. To give as much room as possible in these proceedings to the targeted talks, no presentation of the Very Large Telescope Observatory has been included. All readers missing such a presentation are reminded that up-to­ date in-depth information about the VLT status is available electronically.1 Papers were given concerning observations in the entire electromagnetic spectrum from x-rays to mm-waves, i.e., exceeding 22 octaves in frequency. The VLT as any ground-based optical observatory can only address at best 7 octaves. Nevertheless the VLT, most likely the only ground-based observa­ tory specifically designed to access all these 7 octaves of the electromagnetic spectrum practically in parallel, will undoubtedly be a tool of extreme value to this field.

Editors and Affiliations

  • European Southern Observatory, Garching, Germany

    Hans Ulrich Käufl

  • Villafranca del Castillo, Satellite Tracking Station, ESA, Madrid, Spain

    Ralf Siebenmorgen

Bibliographic Information

  • Book Title: The Role of Dust in the Formation of Stars

  • Book Subtitle: Proceedings of the ESO Workshop Held at Garching, Germany, 11–14 September 1995

  • Editors: Hans Ulrich Käufl, Ralf Siebenmorgen

  • Series Title: ESO Astrophysics Symposia

  • DOI: https://doi.org/10.1007/978-3-540-68594-4

  • Publisher: Springer Berlin, Heidelberg

  • eBook Packages: Springer Book Archive

  • Copyright Information: Springer-Verlag Berlin Heidelberg 1996

  • Softcover ISBN: 978-3-662-22515-8Published: 03 October 2013

  • eBook ISBN: 978-3-540-68594-4Published: 29 June 2013

  • Series ISSN: 1431-2433

  • Series E-ISSN: 1611-6143

  • Edition Number: 1

  • Number of Pages: XXII, 461

  • Topics: Astronomy, Observations and Techniques, Astrophysics and Astroparticles, Geophysics/Geodesy

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