- Page 1 and 2: Max Planck Institute for Astronomy
- Page 3 and 4: Max Planck Institute for Astronomy
- Page 5: Contents Preface ..................
- Page 9 and 10: Galaxies and Cosmology The “Realm
- Page 11 and 12: I.2 Observatories, Telescopes, and
- Page 13 and 14: Instrumentation for Ground-based As
- Page 15 and 16: Fig. I.5: The European he r s c h e
- Page 17 and 18: edshifts z 2, that is, to a look-b
- Page 19 and 20: Edinburgh Hatfield Kopenhagen Durha
- Page 21 and 22: I.4 Teaching and Public Outreach St
- Page 23 and 24: Fig. II.1.2: TW Hydrae’s dust dis
- Page 25 and 26: the circumstellar disk. Subsequentl
- Page 27 and 28: Age [Gyr] 0.25 0.20 0.15 0.10 0.05
- Page 29 and 30: Stars with 50% Completeness 40 30 2
- Page 31 and 32: II.3 Rapid Formation of Planetesima
- Page 33 and 34: max( p )/< g > 1000 100 10 1 0.1 0
- Page 35 and 36: t =4 T orb t =5 T orb Is this then
- Page 37 and 38: normalize by stellar model construc
- Page 39 and 40: The astronomers identified four dom
- Page 41 and 42: II.5 Dwarf Galaxies Under the Magni
- Page 43 and 44: 5 ground galaxies could be excluded
- Page 45 and 46: g [mag] 18 20 22 24 26 -1 -0.5 0 0.
- Page 47 and 48: F [10 -23 W cm -2 nm -1 ] N 15 10
- Page 49 and 50: FeII / MgII unknown interactive rel
- Page 51 and 52: II.7 Dwarf Galaxies - the "Missing
- Page 53 and 54: The Search for Needles in the Hay S
- Page 55 and 56: 0.4 0.2 0 -0.2 -0.4 0.2 0.1 0 -0.1
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Here a comparison between absolute
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very moderately enhanced central de
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M81 Zwerg A Holmberg I Holmberg II
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log( HI /(M pc -2 )), log( H2 /(M
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favored - for example, in dwarf gal
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dwarf and starburst galaxies may of
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Fig. III.1.1: a) The LBT view of th
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(r) 20 15 10 5 0 -5 0 2 4 6 r [kpc]
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III.2 In What Type of Galaxies Do Q
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spectra of quasar and galaxy. As an
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limits because the observed rest wa
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seems consistent with the present v
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III.3 Chemistry in Protoplanetary D
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the freeze-out temperature of CO (2
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Z [AU] 800 600 400 200 200 8.0 400
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ciently small channel widths of 0.1
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we continue our study for other obs
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extinction and crowding due to the
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Outlook Recently, Stolte et al. (20
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mode seeing limited diffrectionlimi
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liquid nitrogen are housed in the l
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The Software The software for Lucif
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Fig. IV.1.11: Installation of the u
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Differential Image Motion Monitor U
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IV.2. Instruments for the VLT Cat's
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Fig. IV.2.3: Schematic view of the
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sph_ifs_ sph_ifs_ MasterBlas Master
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e overcome: For a long time it was
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Fig. IV.3.2.: The design of Panic.
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Fig. IV.4.3: The CCD mosaic of the
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Cryogenic Wheel Mechanisms for the
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V People and Events V.1 Conferences
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V.2 The “Night of Science” For
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V.3 Th i s b e’s Last Journey In
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V.4 Honors, Prizes, and an Appointm
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Anders Johansen, Boris Häussler, a
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Benjamin Moster receives the Univer
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V.5 A Researcher’s Enthusiasm Inf
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In Heidelberg, cooperation between
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Fig. V.6.1: Ranga Yogeshwar standin
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Ranga Yogeshwar was born in Luxembo
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Borelli, Briegel, Kittmann (Guest,
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Friedrich Müller, Markus Nielbock,
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F. Huisken: Member of the Internati
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Arlt Computer, Magstadt Arrow Centr
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SE Spezial-Electronic AG, Bückebur
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disk winds, jets, outflows” (JEts
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Robert Tubbs: VLTI training school
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February 12; “Geheimnisvolle Quas
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an infalling envelope. Astronomy an
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DEEP2 and Combo-17: implications fo
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Körding, E. G., S. Jester, R. Fend
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Najita, T. Henning: The dust, plane
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Sanders, D. B., M. Salvato, H. Auss
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zation of unresolved galaxies for G
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stellar populations. In: Stellar Po
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Instrumentation XV, (Ed.) Strojnik-
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Popular Papers Blum, J., S. Wolf, H
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The Max Planck Society The Max Plan