標題: Titlebook: QSO Hosts and Their Environments; Isabel Márquez,Josefa Masegosa,Josefina Molina Book 2001 Springer Science+Business Media New York 2001 P [打印本頁] 作者: exposulate 時間: 2025-3-21 18:45
書目名稱QSO Hosts and Their Environments影響因子(影響力)
書目名稱QSO Hosts and Their Environments影響因子(影響力)學科排名
書目名稱QSO Hosts and Their Environments網絡公開度
書目名稱QSO Hosts and Their Environments網絡公開度學科排名
書目名稱QSO Hosts and Their Environments被引頻次
書目名稱QSO Hosts and Their Environments被引頻次學科排名
書目名稱QSO Hosts and Their Environments年度引用
書目名稱QSO Hosts and Their Environments年度引用學科排名
書目名稱QSO Hosts and Their Environments讀者反饋
書目名稱QSO Hosts and Their Environments讀者反饋學科排名
作者: PANT 時間: 2025-3-21 23:52 作者: 身體萌芽 時間: 2025-3-22 04:27 作者: 昏迷狀態(tài) 時間: 2025-3-22 04:52 作者: 臆斷 時間: 2025-3-22 12:09
W. J. Percival,L. Miller,R. J. McLure,J. S. Dunlop church became a major concern; the sacraments and church membership became rigidly controlled ends rather than flexible means. The keys to this “kingdom of heaven,” as pointed out in the Heidelberg Catechism,. were the preaching of the Word and the exercise of ecclesiastical discipline..作者: 攀登 時間: 2025-3-22 12:59 作者: 發(fā)酵 時間: 2025-3-22 20:09
Margrethe Wold,Mark Lacy,Per B. Lilje,S. Serjeant church became a major concern; the sacraments and church membership became rigidly controlled ends rather than flexible means. The keys to this “kingdom of heaven,” as pointed out in the Heidelberg Catechism,. were the preaching of the Word and the exercise of ecclesiastical discipline..作者: heart-murmur 時間: 2025-3-22 21:25 作者: capsaicin 時間: 2025-3-23 03:21 作者: 思想流動 時間: 2025-3-23 06:35 作者: 注視 時間: 2025-3-23 11:48
Riccardo Scarpa,C. Megan Urryrary for their never failing courtesy and unwearied assistance. I am also indebted to a number of persons in the Netherlands Ministry of Foreign Affairs, chiefly in the archives division. That their help was not more extensive was not due to unwillingness on their part to be of service. To the University of C978-94-011-6811-3978-94-011-6809-0作者: 叢林 時間: 2025-3-23 17:36
L. Lara,W. D. Cotton,L. Feretti,G. Giovannini,J. M. Marcaide,I. Márquez,T. Venturi to him as examples. I argue that this is particularly true with respect to T.S. Eliot. Tracing the relationship of Nijhoff to Eliot allows us to situate Nijhoff in a wider-than-Dutch-modernist-literary context, and with him Dutch interbellum literature.作者: 交響樂 時間: 2025-3-23 18:27 作者: affluent 時間: 2025-3-23 23:20 作者: alliance 時間: 2025-3-24 05:12
Knud Jahnke,Bj?rn Kuhlbrodt,Eva ?rndahl,Lutz Wisotzkis, boxes, book-covers, beakers, tankards, cups, bowls, basins, bottles, plate used for the toilet, for the table, candlesticks and plate used for the service of tea, coffee and chocolate. A general survey of a number of objects is given in the Introductions to the first and second volumes (Volume I, p. VI; Vo978-94-010-3662-7作者: 招致 時間: 2025-3-24 09:58
Jary K. Kotilainen,Renato Falomobook-covers, beakers, tankards, cups, bowls, basins, bottles, plate used for the toilet, for the table, candlesticks and plate used for the service of tea, coffee and chocolate. A general survey of a number of objects is given in the Introductions to the first and second volumes (Volume I, p. VI; Vo作者: 油膏 時間: 2025-3-24 13:24 作者: forthy 時間: 2025-3-24 18:00
Isabel Márquez,Patrick Petitjean,Bertrand Theodore,Malcolm Bremer,Guy Monnet,Jean-Luc Beuzit作者: 變色龍 時間: 2025-3-24 20:24 作者: 樹上結蜜糖 時間: 2025-3-24 23:44
Book 2001d evolution. This volume provides a valuable overview and timely update of the exciting and rapidly developing field of QSO hosts and their environments - essential reading for graduate students and researchers.作者: 強壯 時間: 2025-3-25 05:06
rmation and evolution. This volume provides a valuable overview and timely update of the exciting and rapidly developing field of QSO hosts and their environments - essential reading for graduate students and researchers.978-1-4613-5199-3978-1-4615-0695-9作者: Fantasy 時間: 2025-3-25 10:24
978-1-4613-5199-3Springer Science+Business Media New York 2001作者: 細頸瓶 時間: 2025-3-25 13:01 作者: Mere僅僅 時間: 2025-3-25 17:17
The Real Difference Between Radio-Loud and Radio-Quiet AGNsoud and radio-quiet AGNs. It is quite clear that the real difference between these two classes is the JET. So the discussion should be: why some AGNs have a powerful radio jet and some other don’t have. I will briefly discuss about the possible explanations for this fundamental difference.作者: allude 時間: 2025-3-25 23:51 作者: 難解 時間: 2025-3-26 02:08
Three Peculiar Objects From a New Sample of Radio Galaxiesabove +60°, total flux density greater than 100 mJy at 1.4 GHz and angular size larger then 4′ have been selected and observed with the VLA at 1.4 and 4.9 GHz. A number of peculiar radio galaxies have been discovered, of which we present here results on J1835+620, J2114+820 and J2157+664.作者: set598 時間: 2025-3-26 07:53
The Luminosity Function of QSO Host GalaxiesSO hosts is similar in shape to that of normal galaxies, although offset in normalisation by a factor of 10.. This supports the hypothesis that the parent population of quasars is identical to the general population of early-type field galaxies.作者: 過多 時間: 2025-3-26 09:03
http://image.papertrans.cn/q/image/780023.jpg作者: LASH 時間: 2025-3-26 13:22 作者: Cabg318 時間: 2025-3-26 19:59
Associated Absorption and Radio Source GrowthEvidence is presented that C IV associated absorption is seen preferentially towards steep-spectrum radio sources of small linear size. A model for the clearing out of absorbing gas along the jet axis as the radio source grows is proposed. The general properties of the absorbers suggest that AGN environments are gas-rich.作者: Amplify 時間: 2025-3-27 00:12 作者: carotenoids 時間: 2025-3-27 01:57 作者: 受人支配 時間: 2025-3-27 08:09 作者: Alopecia-Areata 時間: 2025-3-27 09:51 作者: 跑過 時間: 2025-3-27 13:37 作者: intelligible 時間: 2025-3-27 18:16
The Hosts Galaxies of Radio-Loud and Radio-Quiet Quasarsxt of the general galaxy population. It is now clear that the hosts of radio-loud . radio-quiet quasars with . . < ?23.5 are virtually all massive elliptical galaxies. The masses of these spheroids are as expected given the relationship between black-hole and spheroid mass found for nearby quiescent作者: 噴油井 時間: 2025-3-27 23:54
The Nucleus-Host Galaxy Connection in Radio-Loud AGNconsists of 57 objects, divided into sub-samples of 40 BL Lac objects and 17 RL quasars. Essentially all the AGN nuclei lie in luminous elliptical galaxies (Es), which follow the Kormendy relation for normal Es. The host galaxies occupy a narrow range of ~1 magnitude, compared to >5 orders of magnit作者: 大酒杯 時間: 2025-3-28 02:07 作者: outset 時間: 2025-3-28 07:43
The Radio Loudness Dichotomy: Environment or Black-Hole Mass?asars are presented. No evidence is found for a difference in large-scale environments, with both quasar classes found to be located in clusters of Abell class ~ 0. Conversely, virial black-hole mass estimates based on H. line-widths show a clear difference in the quasar black-hole mass distribution作者: radiograph 時間: 2025-3-28 13:38
QSO Environments at Intermediate Redshifts Our observations include images of background control fields to provide a good determination of the field galaxy counts. About 10 per cent of the quasars appear to live in rich clusters, whereas approximately 45 per cent live in environments similar to that of field galaxies..The richness of galaxi作者: 千篇一律 時間: 2025-3-28 17:55
Host Galaxies and Cluster Environment of BL Lac Objects at , > 0.5ain aim of this study is to confirm the apparent evolution previously claimed. A host galaxy was detected in all BL Lac objects at . < 0.7. At higher redshifts our search was not successful. An exception might be PKS 0426–380 (z > 1.03). Here we detected a galaxy, which might be either along the lin作者: 不可接觸 時間: 2025-3-28 21:56 作者: 減至最低 時間: 2025-3-29 02:40
The Real Difference Between Radio-Loud and Radio-Quiet AGNsoud and radio-quiet AGNs. It is quite clear that the real difference between these two classes is the JET. So the discussion should be: why some AGNs have a powerful radio jet and some other don’t have. I will briefly discuss about the possible explanations for this fundamental difference.作者: enterprise 時間: 2025-3-29 05:14
Broadband Optical Colours of Intermediate Redshift QSO Host Galaxiestical comparison between radio-loud and radio-quiet objects, we selected pairs of objects with approximately the same redshift and V-magnitude. Data was obtained in 1994 at the ESO NTT and at the Nordic Optical Telescope, primarily in the R band, but some of them also in V and/or I.作者: ineluctable 時間: 2025-3-29 07:40 作者: Gnrh670 時間: 2025-3-29 11:48 作者: intelligible 時間: 2025-3-29 17:32 作者: 繁榮地區(qū) 時間: 2025-3-29 21:05 作者: pericardium 時間: 2025-3-30 00:47 作者: grudging 時間: 2025-3-30 06:12 作者: 小畫像 時間: 2025-3-30 09:59
The Host Galaxies of Luminous Radio-Quiet Quasars suggested from studies of lower nuclear luminosity quasars and Seyfert galaxies. We show how simple theoretical models of quasar activity predict such a limit, and suggest how this picture must be changed in light of our results.作者: Critical 時間: 2025-3-30 13:19 作者: Retrieval 時間: 2025-3-30 20:02
QSO Environments at Intermediate Redshiftsature, we find no evidence of an evolution in the environment with epoch. Instead, a weak, but significant correlation between quasar radio luminosity and environmental richness is present. It is thus possible that the environments of quasars, at least the powerful ones, do not evolve much between the present epoch and . ≈ 0.8.作者: Countermand 時間: 2025-3-31 00:16 作者: coalition 時間: 2025-3-31 01:12 作者: fastness 時間: 2025-3-31 06:49
Adaptive-Optics Imaging of Low and Intermediate Redshift Quasarseveal bars and spiral arms. The morphology of the other objects are difficult to determine from one dimensional fit to the host galaxies; deeper images are needed..Analysis of mocked data shows that elliptical galaxies are always recognized as such, whereas disk hosts can be missed for small disk scale lengths and large QSO contributions.作者: MONY 時間: 2025-3-31 12:25
The Radio Loudness Dichotomy: Environment or Black-Hole Mass?s. Our results suggest that a black-hole mass of ~ 10. M. is required to produce a powerful radio-loud quasar, and that it is black-hole mass and accretion rate which hold the key to the radio-loudness dichotomy.作者: crockery 時間: 2025-3-31 15:25 作者: Assemble 時間: 2025-3-31 17:41
