標題: Titlebook: Dense Molecular Gas around Protostars and in Galactic Nuclei; European Workshop on W.A. Baan,Y. Hagiwara,H.J. Langevelde Book 2005 Springer [打印本頁] 作者: 叛亂分子 時間: 2025-3-21 18:25
書目名稱Dense Molecular Gas around Protostars and in Galactic Nuclei影響因子(影響力)
書目名稱Dense Molecular Gas around Protostars and in Galactic Nuclei影響因子(影響力)學(xué)科排名
書目名稱Dense Molecular Gas around Protostars and in Galactic Nuclei網(wǎng)絡(luò)公開度
書目名稱Dense Molecular Gas around Protostars and in Galactic Nuclei網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Dense Molecular Gas around Protostars and in Galactic Nuclei被引頻次
書目名稱Dense Molecular Gas around Protostars and in Galactic Nuclei被引頻次學(xué)科排名
書目名稱Dense Molecular Gas around Protostars and in Galactic Nuclei年度引用
書目名稱Dense Molecular Gas around Protostars and in Galactic Nuclei年度引用學(xué)科排名
書目名稱Dense Molecular Gas around Protostars and in Galactic Nuclei讀者反饋
書目名稱Dense Molecular Gas around Protostars and in Galactic Nuclei讀者反饋學(xué)科排名
作者: Blatant 時間: 2025-3-21 21:23
Domain-Specific Languages in Practiceeakage for the evolution of cloud cores; (iii) the phase of anisotropic dynamical collapse following the formation of strongly peaked density distributions; (iv) the mechanism of magnetic braking as a possible solution to the angular momentum problem in star formation.作者: ELATE 時間: 2025-3-22 00:30 作者: 沉思的魚 時間: 2025-3-22 07:56 作者: 尾巴 時間: 2025-3-22 09:55 作者: exophthalmos 時間: 2025-3-22 12:55 作者: exophthalmos 時間: 2025-3-22 17:54 作者: 戰(zhàn)役 時間: 2025-3-22 22:09 作者: nerve-sparing 時間: 2025-3-23 02:35 作者: 啤酒 時間: 2025-3-23 08:44
Magnetic Fields in Star-Forming Regions: Theoretical Aspectseakage for the evolution of cloud cores; (iii) the phase of anisotropic dynamical collapse following the formation of strongly peaked density distributions; (iv) the mechanism of magnetic braking as a possible solution to the angular momentum problem in star formation.作者: STENT 時間: 2025-3-23 12:31
VLBI Water Maser Proper Motion Measurements in Star-Forming Regionst scales of AUs, discovering new phenomena (e.g., isotropic mass ejections, watermaser “micro-structures” exhibiting remarkable coherent and well ordered spatio-kinematical behavior at AU scale), and opening new, puzzling questions related to the early stellar evolution.作者: 兩棲動物 時間: 2025-3-23 17:24 作者: 敘述 時間: 2025-3-23 18:20
H20 Megamasers: Accretion Disks, Jet Interaction, Outflows or Massive Star Formation?r jets with dense molecular gas and to investigate the circumnuclear environment of active galactic nuclei (AGN). Accretion disks with radii of 0.1–3 pc were mapped and masses of nuclear engines of order 10.–10. .? were determined. So far, ～50 extragalactic H.0 maser sources have been detected, but few have been studied in detail.作者: Irritate 時間: 2025-3-24 01:22
A Molecular Ring in the Liner NGC 5218 the inner 500 pc. The SFR is 2–3 . yr . and the SFE is ～13, which are low or moderate values for that gas surface density. We interpret the inner feature as a rotating molecular ring with a radius of ～200 pc. We furthermore suggest that the LINER activity in NGC 5218 is not caused by an aging starburst, but by a buried AGN.作者: 極端的正確性 時間: 2025-3-24 05:26 作者: hallow 時間: 2025-3-24 07:44
Engineering Gameful Applications with MPSe within 60 mas and in velocity within 0.3 km s. in both targets implying that both maser transitions arise from the same region. According to the modelling by Gray [MNRAS 252 (1991) 30] the 1720/4765-MHz co-propagation requires a low density, warm environment. The masers lie at the edges of H II regions where such conditions are expected.作者: palpitate 時間: 2025-3-24 10:45 作者: AIL 時間: 2025-3-24 16:52
MERLIN and Puschino Observations of H2O Masers in Outer Galactic SFR S128Nrift velocity variations this suggests that the masers trace the dissipation of supersonic turbulence. The spatial distribution of velocities shows that this is in parts more structured than the Kolmogorov cascade.作者: impaction 時間: 2025-3-24 19:54
Leisure Studies in a Global Eraa molecular outflow near the plane of the sky. Ammonia emission is extended and anticorrelated with CCS. We have detected for the first time this anticorrelation at small scales (1400 AU) in a star-forming region.作者: 幻影 時間: 2025-3-25 01:20
https://doi.org/10.1057/9781137415547ch exhibit the “fractal fashion” and express turbulence on very small scales. Together, we have demonstrated that observations of water masers enable us to comprehensively enhance our understanding of the early stages of the formation of massive stars in clusters.作者: 救護車 時間: 2025-3-25 05:02
Clinton L. Beckford,Donovan R. Campbellspots are most likely associated with the tangentially seen parts of a nuclear accretion disk, while an association with dense warm gas interacting with the radio jets cannot yet be ruled out entirely.作者: 修飾 時間: 2025-3-25 07:53
Domestic Homicides and Death Reviewst evolution. The discussion on the interpretation of HNC 1-0 emission includes the importance of ion-neutral chemistry in a luminous starburst region. Finally, simple cartoon ISM models and how they can be applied to LIRGs and ULIRGs, are presented.作者: dearth 時間: 2025-3-25 14:59 作者: 上流社會 時間: 2025-3-25 15:48 作者: Inculcate 時間: 2025-3-25 21:25 作者: 偏見 時間: 2025-3-26 03:19 作者: labile 時間: 2025-3-26 05:44
Outflow, Infall, and Rotation in High-Mass Star Forming Regionsn pressure should reverse the infall thus preventing further growth of the stellar mass. After illustrating the two models proposed to solve this problem (“accretion” and “coalescence”), we review the observational evidence pro/contra such models, focusing on the kinematics of the molecular gas wher作者: 比目魚 時間: 2025-3-26 10:33
MERLIN and Puschino Observations of H2O Masers in Outer Galactic SFR S128N from the Puschino radio telescope. The drift velocities of the masers and the velocity and location of a new maser region add depth to the model of two colliding CO clouds triggering collapse. Some H.O masers appear to originate directly from this shock front. The brightest maser appears typical of作者: ineptitude 時間: 2025-3-26 16:09 作者: Fretful 時間: 2025-3-26 17:25 作者: 蛤肉 時間: 2025-3-26 23:54 作者: 信徒 時間: 2025-3-27 01:31 作者: 不舒服 時間: 2025-3-27 07:47
High-Resolution Observations in B1-IRS: Ammonia, CCS and Water Masers high angular resolution (～4″). We have used VLA observations of NH., CCS, and H.O masers at 1 cm. CCS emission shows three clumps around the central source, with a velocity gradient from red to blue-shifted velocities towards the protostar, probably due to the interaction with outflowing material. 作者: Aromatic 時間: 2025-3-27 12:11 作者: 好開玩笑 時間: 2025-3-27 15:00
Gravitationally Induced Inflow in Starbursts and AGNars. There is also convincing evidence for relations between the properties of supermassive black holes in the nuclei of galaxies and those of their host galaxies. It is much less clear, however, how stellar starburstt) and non-stellar (AGN) activity in the nuclear regions can be initiated and fuell作者: ellagic-acid 時間: 2025-3-27 18:31
Feeding Monsters — A Study of Active Galaxiesr resolution and high sensitivity carried out with the IRAM Plateau de Bure interferometer (PdBI). The observations cover galaxies in a redshift range of ～0.03–1.4. We have so far observed five different active galaxies: NGC3718, NGC1068, HE1029-1831, 3C48 and Q0957 + 561. The first two objects belo作者: EVEN 時間: 2025-3-28 00:49
The QSO Hosts I Zw 1 and 3C 48: Prototypes of a Merger-Driven Quasar Evolution?rared galaxies (ULIRGs) to quasi-stellar objects (QSOs). Since galaxy mergers are assumed to trigger the evolution, it is important to confirm the merger properties of transitionary objects. Using multi-wavelength observations and N-body simulations, the merger histories of I Zw 1 and 3C 48 have bee作者: cancellous-bone 時間: 2025-3-28 02:42 作者: 是突襲 時間: 2025-3-28 07:14 作者: Corporeal 時間: 2025-3-28 12:55
Dense Gas, Chemistry and Star Formation in Luminous Galaxiestution of the molecular gas will change with, and respond to, the evolution of the activity. This paper includes a short discussion of the .CO/.CO 1-0 line intensity ratio as a diagnostic tool of the molecular gas properties of luminous galaxies — paired with examples of high-resolution studies of h作者: Conserve 時間: 2025-3-28 15:08
A Molecular Ring in the Liner NGC 5218entration with extensions out to a radius of 12″. The molecular mass detected is 2.4 × 10. . and the gas surface density is high, ～3000 . pc square in the inner 500 pc. The SFR is 2–3 . yr . and the SFE is ～13, which are low or moderate values for that gas surface density. We interpret the inner fea作者: Lobotomy 時間: 2025-3-28 20:15 作者: TERRA 時間: 2025-3-29 00:57
discussed here are often in an early stage and undoubtedly their progress has bene?ted greatly from the opportunity to discuss results with the experts in a wide range of areas. Similarly, we feel con?dent tha978-90-481-6772-2978-1-4020-3831-0作者: 襲擊 時間: 2025-3-29 03:52
Domestic Dog Cognition and Behavior activity. The overall lack of observational evidence for direct causal relationships between the presence of bars and interactions on the one hand, and starburst or Seyfert activity on the other could, however, easily be due to the possibility that we are not yet considering the correct spatial- or作者: myocardium 時間: 2025-3-29 10:37
https://doi.org/10.1007/978-3-642-53994-7ibution caused by orbit crowding effects. Based on these new data we have improved recent simulations of the warped disk in NGC3718. HE1029-1831 and 3C48 are nearby QSOs. HE10297-1831 is taken out of the Cologne nearby QSO sample. The maps of the integrated CO(1-0) and CO(2–1) emission clearly show 作者: 脾氣暴躁的人 時間: 2025-3-29 11:46
EVN Observations of H2O Masers Towards the High-Mass Young Stellar Object in AFGL 5142作者: 潛伏期 時間: 2025-3-29 15:42
Dense Molecular Gas around Protostars and in Galactic NucleiEuropean Workshop on作者: Invertebrate 時間: 2025-3-29 19:42
Dense Molecular Gas around Protostars and in Galactic Nuclei978-1-4020-3831-0作者: infinite 時間: 2025-3-30 03:06
Gravitationally Induced Inflow in Starbursts and AGN activity. The overall lack of observational evidence for direct causal relationships between the presence of bars and interactions on the one hand, and starburst or Seyfert activity on the other could, however, easily be due to the possibility that we are not yet considering the correct spatial- or作者: 盡忠 時間: 2025-3-30 05:16 作者: fiction 時間: 2025-3-30 09:50 作者: 邊緣帶來墨水 時間: 2025-3-30 14:33 作者: Endoscope 時間: 2025-3-30 20:33 作者: emission 時間: 2025-3-30 22:36
Nicholas Roussopoulos,Wilfrid Utzn pressure should reverse the infall thus preventing further growth of the stellar mass. After illustrating the two models proposed to solve this problem (“accretion” and “coalescence”), we review the observational evidence pro/contra such models, focusing on the kinematics of the molecular gas wher作者: PRO 時間: 2025-3-31 04:01
Nicholas Roussopoulos,Wilfrid Utz from the Puschino radio telescope. The drift velocities of the masers and the velocity and location of a new maser region add depth to the model of two colliding CO clouds triggering collapse. Some H.O masers appear to originate directly from this shock front. The brightest maser appears typical of作者: NATAL 時間: 2025-3-31 07:26
https://doi.org/10.1007/978-3-030-73758-0ervational method favours different regimes of scale size, density and other physical conditions. The available techniques and their ranges of applicability are briefly described and the current status of observations is reviewed, with particular emphasis on high-resolution observations of star-form作者: inchoate 時間: 2025-3-31 09:33 作者: MELD 時間: 2025-3-31 14:32 作者: 錫箔紙 時間: 2025-3-31 18:20 作者: 古董 時間: 2025-4-1 00:51 作者: 有害 時間: 2025-4-1 05:50
https://doi.org/10.1057/9781137415547otions exhibit outflows, which likely originate from two of the hyper-compact HII regions in this source. Sarma et al., have detected the Zeeman effect in water masers toward W3 IRS5 and measured line-of-sight magnetic field strengths of between 14 and 42 mG. The directions of maser linear polarizat作者: esthetician 時間: 2025-4-1 08:53
Domestic Dog Cognition and Behaviorars. There is also convincing evidence for relations between the properties of supermassive black holes in the nuclei of galaxies and those of their host galaxies. It is much less clear, however, how stellar starburstt) and non-stellar (AGN) activity in the nuclear regions can be initiated and fuell作者: constellation 時間: 2025-4-1 10:55 作者: 冥界三河 時間: 2025-4-1 17:32 作者: remission 時間: 2025-4-1 21:01
Clinton L. Beckford,Donovan R. Campbellngle-dish monitoring and high-resolution interferometry have been used to identify sites of massive star formation, to study the interaction of nuclear jets with dense molecular gas and to investigate the circumnuclear environment of active galactic nuclei (AGN). Accretion disks with radii of 0.1–3 作者: Condense 時間: 2025-4-2 02:08
Clinton L. Beckford,Donovan R. Campbelled as a part of a small sample of FR II galaxies with evidence of nuclear obscuration. The isotropic luminosity of the maser is ～1200 .?. With a recessional velocity of cz ～- 17680 km s. it is the most distant water maser so far reported. The line arises from the densest (>10. cm .) interstellar gas作者: Charade 時間: 2025-4-2 02:51 作者: 改變立場 時間: 2025-4-2 10:00
