Werner Behrendt; Ulrich W. Gerwarth; Reinhard Haubold; Jörn v. Jouanne; Jörn Jouanne; Hannelore Keller-Rudeck; Keller-Rude Springer-Verlag Berlin and Heidelberg GmbH & Co. KG (2013) Pehmeäkantinen kirja
Hannelore Keller-Rudek; Dieter Koschel; Peter Merlet; Ulrike Ohms-Bredemann; Joachim Wagner; Astrid Wietelmann Springer-Verlag Berlin and Heidelberg GmbH & Co. KG (1992)
Werner Behrendt; Ulrich W Gerwarth; Reinhard Haubold; Jarn V Jouanne; Hannelore Keller-Rudeck; Dieter Koschel; Ha Schafer Springer-Verlag Berlin and Heidelberg GmbH & Co. KG (1994)
Walter Hack; Reinhard Haubold; Claudia Heinrich-Sterzel; Hannelore Keller-Rudek; Ulrike Ohms-Bredemann; Dag Schiaberg; Str Springer-Verlag Berlin and Heidelberg GmbH & Co. KG (1993)
Reinhard Haubold; Jarn V Jouanne; Hannelore Keller-Rudek; Peter Merlet; Ulrike Ohms-Bredemann; Carol Strametz; Joa Wagner Springer-Verlag Berlin and Heidelberg GmbH & Co. KG (1991)
Norbert Baumann; Hans Jurgen Fachmann; Brigitte Heibel; Hannelore Keller-Rudek; Alfons Kubny Springer-Verlag Berlin and Heidelberg GmbH & Co. KG (1987)
This volume C 1 is the first supplement volume to "Phosphor" C which was published in 1965 and covers the compounds of phosphorus. Starting with the binary species formed between phosphorus and hydrogen, the present volume deals with the neutral mononuclear compounds PH through PH ; the ions featuring the same stoichiometric composition are s covered in separate sections. PH and PH are the major initial gaseous decomposition products of PH and, thus, also 2 J intermediates in many of its gas-phase reactions. Both molecules and their ions have been thoroughly investigated by a variety of modern, high-resolution spectroscopic methods during the last three decades. The coverage of their physical, and mostly molecular, properties re presents the largest part of the first two chapters (PH and ions pp. 2 to 47; PH and ions pp. 47 2 to 111). PH is the only compound described in this volume which is thermally stable under normal J conditions. It is the phosphorus analog of ammonia, but exhibits, however, a quite different chemical behavior towards most elements and compounds. The majority of its physical, and in particular spectroscopic, properties have been determined in great detail since the sixties, partially in regard to spectroscopic investigations of the atmospheres of the outer planets.