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標(biāo)題: Titlebook: A Few Tens au Scale Physical and Chemical Structures Around Young Low-Mass Protostars; Yoko Oya Book 2022 Springer Nature Singapore Pte Lt [打印本頁]

作者: 宗派    時(shí)間: 2025-3-21 16:57
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作者: choroid    時(shí)間: 2025-3-21 20:55

作者: compel    時(shí)間: 2025-3-22 00:29
Air Lubricated and Air Cavity Shipslight its centrifugal barrier. Moreover, some molecular lines trace disk components even inside the centrifugal barrier. This chapter discusses chemical processes to cause the chemical diversity and the chemical differentiation.
作者: 整潔    時(shí)間: 2025-3-22 06:38
https://doi.org/10.1007/978-3-642-65563-0ns. As for the outflow components, a parabolic model is employed. The details of these models are described in this chapter. Moreover, some representative examples of the model results are presented to demonstrate their dependences of the kinematic structure on the physical parameters.
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作者: AGGER    時(shí)間: 2025-3-23 03:31
,IRAS 16293–2422 Source A,peals to palliative care providers, hematologists, oncologists, psychiatrists, nurses and health professionals as well as researchers, academics, policy-makers, and social scientists working in health care. It 978-3-030-56794-1978-3-030-56795-8
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作者: 使混合    時(shí)間: 2025-3-23 11:57
Introduction,ulated. However, the change in mind came too late for the Presidential Elections of 2016, won by the green candidate Van der Bellen but just in time for a governmental coalition with the Conservative party (?VP) in 2017, signing up to a pro-European coalition agreement.
作者: 招人嫉妒    時(shí)間: 2025-3-23 15:17

作者: 影響深遠(yuǎn)    時(shí)間: 2025-3-23 22:01
Model Calculation, book, analysis brings these interlinked tensions to light, exploring the roles of culture and identity, alongside and a productive conversation with the political and economic projects of post-war European integration.?978-981-13-9429-4978-981-13-9427-0
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作者: Salivary-Gland    時(shí)間: 2025-3-24 04:13
,IRAS 15398–3359,l phase than they are afraid of dying itself. When polled, most Americans tell us they would prefer to die at home, surrounded by loved ones, rather than in a hospital receiving high-tech tests and treatments until the last. Yet the majority of people, even those with term- inal illnesses, die in th
作者: Adrenaline    時(shí)間: 2025-3-24 08:16

作者: AROMA    時(shí)間: 2025-3-24 11:26
L483,ozooplankton release NH., urea, and amino acids by direct excretion and by ‘sloppy feeding’, but they also control both the rates of nitrogen regeneration and uptake within the community by grazing the microzooplankton, the primary regenerators of NH., and the phytoplankton, the primary consumers of
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作者: Reverie    時(shí)間: 2025-3-24 21:02

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作者: 混雜人    時(shí)間: 2025-3-25 04:01

作者: 細(xì)頸瓶    時(shí)間: 2025-3-25 08:53
A Few Tens au Scale Physical and Chemical Structures Around Young Low-Mass Protostars
作者: daredevil    時(shí)間: 2025-3-25 14:16
https://doi.org/10.1007/978-3-642-65563-0(. au) outflow based on the .CO (.) observation, and to the morphology of infrared reflection near the protostar (. au). The discrepancy with the infrared observation result could originate from high extinction by the outflow cavity on the western side. Alternatively, these discrepancies may indicat
作者: nullify    時(shí)間: 2025-3-25 16:34
Johanan H. Odhner,Robert J. Levis, the radius of the centrifugal barrier does not. This is the first indication of the centrifugal barrier of the infalling-rotating envelope in a hot corino source. CH.OH and HCOOCH. may be liberated from ice mantles due to weak accretion shocks around the centrifugal barrier and/or due to protostel
作者: 怕失去錢    時(shí)間: 2025-3-25 22:59
Air Lubrication and Air Cavity Analysis,s is roughly explained by a simple ballistic model with the protostellar mass from 0.1 to 0.2 . and the radius of the centrifugal barrier from 30 to 200 au by assuming a nearly edge-on geometry with the inclination angle of 80.. The line emissions detected with broad velocity widths most likely come
作者: 歡樂中國    時(shí)間: 2025-3-26 01:54

作者: seroma    時(shí)間: 2025-3-26 06:22
Introduction,ingdom, the support for Austria’s membership of the European Union (EU) increased further. While in April 2016—according to data of the Austria Society for European Politics—60 percent of Austrians wanted their country to stay in the EU, from July 2016 onwards the number of supporters grew to 77 per
作者: 緊張過度    時(shí)間: 2025-3-26 10:59

作者: Mendicant    時(shí)間: 2025-3-26 15:19
Model Calculation,Europe.Explores the role of culture and identity in post-warThis book uses the Eurovision Song Contest (ESC), as an analytical entry point to understand and illuminate post-War Europe and the drive to create an identity that can legitimise the European project in its broadest sense. The ESC presents
作者: GAVEL    時(shí)間: 2025-3-26 20:21
L1527,st es, wenn dies, wie hier geschehen, sich im Abstand von fast fünfzig Jahren wiederholt. Die Anregung der Stadt Euskirchen zur Wiederholung der ursprünglichen ?Euskirchen-Studie“wurde wegen der ausgesprochen seltenen Chance aufgegriffen, den sozialen Wandel in einer deutschen Mittelstadt durch den
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作者: 拋棄的貨物    時(shí)間: 2025-3-27 12:30
L483,s been little appreciation to date of the interactions between top-down (grazing) control and bottom-up (nutrient supply) control on the structure and nutrient cycling processes within these webs. The quality of nutrient supply, both in terms of the relative proportion of inorganic: organic nitrogen
作者: instructive    時(shí)間: 2025-3-27 14:00

作者: Oration    時(shí)間: 2025-3-27 19:52

作者: 古文字學(xué)    時(shí)間: 2025-3-27 22:01

作者: 柏樹    時(shí)間: 2025-3-28 02:11
Back Mattered between Sweden and Denmark) were used to illustrate basic principles and processes related to nutrient fluxes. We have applied a process-based mass-balance model, CoastMab, to the Kattegat and quantified the nutrient fluxes to, within, and from the system. Several scenarios aiming to decrease eut
作者: 震驚    時(shí)間: 2025-3-28 06:45
A Few Tens au Scale Physical and Chemical Structures Around Young Low-Mass Protostars978-981-19-1708-0Series ISSN 2190-5053 Series E-ISSN 2190-5061
作者: Ointment    時(shí)間: 2025-3-28 13:29
Flight Planning and Management,h the aid of simple kinematic models of the infalling-rotating envelope, Keplerian disk, and the outflow. This study has made some significant contributions to astrochemistry and star-formation studies. The new insights obtained in this thesis also raise new important questions to be addressed in the future.
作者: 致詞    時(shí)間: 2025-3-28 16:59
Roger Gariepy M.D., F.R.C.S. (C)The observational data with Atacama Large Millimeter/submillimeter Array (ALMA) is utilized to study physical and chemical structures of low-mass protostellar sources in the following chapters. This chapter describes the principles of an aperture synthesis with an interferometer and the basic features of ALMA.
作者: 商議    時(shí)間: 2025-3-28 22:45
Yoko OyaNominated as an outstanding Ph.D. thesis by the Department of Physics at the University of Tokyo.Presents simplified models which clearly describe well the disk.Shares a unified picture of chemical di
作者: 噱頭    時(shí)間: 2025-3-29 02:53

作者: Geyser    時(shí)間: 2025-3-29 06:06
Femoral Neck and Femoral Shaft Surgery,ss of the Universe, they form rich structures in the Universe from large scales (clusters of galaxies and galaxies) to small scales (stars and planets). Among such hierarchical structure, stars are the most fundamental physical elements in the Universe. They also play important roles in chemical evo
作者: 擁護(hù)    時(shí)間: 2025-3-29 07:37

作者: 錯(cuò)    時(shí)間: 2025-3-29 12:31
https://doi.org/10.1007/978-3-642-65563-0tacama Large Millimeter/submillimeter Array. The observed lines are investigated to characterize the geometrical configuration of the outflow/envelope system of this source. The CS emission traces both an envelope component extending along the north-south direction and a faint outflow component with
作者: Endoscope    時(shí)間: 2025-3-29 19:14
https://doi.org/10.1007/978-3-642-65563-0oud with Atacama Large Millimeter/Submillimeter Array. A compact component concentrated in the vicinity of the protostar has been detected as well as a well-collimated outflow cavity extending along the northeast-southwest axis. The inclination angle of the outflow is found to be about . based on th
作者: 改革運(yùn)動(dòng)    時(shí)間: 2025-3-29 22:32

作者: 群居動(dòng)物    時(shí)間: 2025-3-30 03:55
https://doi.org/10.1007/978-3-319-65220-7. A clear chemical differentiation is seen; OCS and H.CS show an extended distribution with a slight rotation signature, while CH.OH and HCOOCH. are concentrated near the protostar. The extended component is interpreted by the infalling-rotating envelope model with a nearly face-on configuration. Th
作者: 得罪    時(shí)間: 2025-3-30 05:20

作者: inveigh    時(shí)間: 2025-3-30 11:36

作者: Endearing    時(shí)間: 2025-3-30 15:17
https://doi.org/10.1007/978-3-031-52994-8nd outflow models described in Chap. .. The physical parameters, such as the protostllar mass, the radius of the centrifugal barrier, and the inclination angle have been derived. In these analyses, the common existence of a centrifugal barrier in the protostellar sources is confirmed. Its physical r




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