Search Results - (Author, Cooperation:P. D'Alessio)
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1C. Qi ; K. I. Oberg ; D. J. Wilner ; P. D'Alessio ; E. Bergin ; S. M. Andrews ; G. A. Blake ; M. R. Hogerheijde ; E. F. van Dishoeck
American Association for the Advancement of Science (AAAS)
Published 2013Staff ViewPublication Date: 2013-07-23Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
2J. J. Tobin ; L. Hartmann ; H. F. Chiang ; D. J. Wilner ; L. W. Looney ; L. Loinard ; N. Calvet ; P. D'Alessio
Nature Publishing Group (NPG)
Published 2012Staff ViewPublication Date: 2012-12-12Publisher: Nature Publishing Group (NPG)Print ISSN: 0028-0836Electronic ISSN: 1476-4687Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsPublished by: -
3D'Alessio, P. ; Wilner, D. J. ; Ho, P. T. P. ; Torrelles, J. M. ; Curiel, S. ; Gómez, Y. ; Lizano, S. ; Pedlar, A. ; Cantó, J. ; Raga, A. C. ; Rodríguez, L. F.
[s.l.] : Macmillan Magazines Ltd.
Published 1998Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Planet formation is believed to occur in the disks of gas and dust that surround young solar-type stars. Most stars, however, form in multiple systems, where the presence of a close companion could affect the structure of the disk and perhaps interfere with planet formation. It has been ...Type of Medium: Electronic ResourceURL: -
4Staff View
ISSN: 1572-946XSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract This paper discusses the formation of two-shock working surfaces in Herbig-Haro (HH) jets. These working surfaces can be formed either at the leading edge of the jet flow, or inside the body of the jet beam (as a result of variabilities in the jet flow velocity), and depending on the parameters of the flow can be either massless or mass conserving. It is shown that observations might indicate that these two regimes actually occur in some HH jets.Type of Medium: Electronic ResourceURL: