派博傳思國際中心

標題: Titlebook: BL Lac Objects; Proceedings of a Wor L. Maraschi,T. Maccacaro,M. -H. Ulrich Conference proceedings 1989 Springer-Verlag Berlin Heidelberg 1 [打印本頁]

作者: 小故障    時間: 2025-3-21 19:47
書目名稱BL Lac Objects影響因子(影響力)




書目名稱BL Lac Objects影響因子(影響力)學科排名




書目名稱BL Lac Objects網絡公開度




書目名稱BL Lac Objects網絡公開度學科排名




書目名稱BL Lac Objects被引頻次




書目名稱BL Lac Objects被引頻次學科排名




書目名稱BL Lac Objects年度引用




書目名稱BL Lac Objects年度引用學科排名




書目名稱BL Lac Objects讀者反饋




書目名稱BL Lac Objects讀者反饋學科排名





作者: 笨拙的你    時間: 2025-3-21 22:33
Statistics of superluminal sources,orentz factor, the Doppler boost exponent and the . exponent, . peaks at a few degrees, well inside the angle for maximum apparent transverse velocity. Theoretical distributions of the apparent transverse velocity are sharply peaked near the maximum possible value, but the observed distribution is p
作者: Flavouring    時間: 2025-3-22 00:30
,The host galaxy of BL Lac objects or what’s in a name?,ontains mostly medium bright radio galaxies. This analysis leads us to suggest that radio galaxies such as those of the B2 bright sample form the parent population of nearby BL Lac objects. Confirmation of this model requires the identification and observation of a larger number of nearby BL Lac obj
作者: Crepitus    時間: 2025-3-22 06:39
A spectroscopic study of blazars at medium resolution. Observations of PKS 0521-36, PKS 0537-44 andizable sample of objects through detection of weak spectral features, either in emission or in absorption; .) monitoring intensity and profile of the broad emission fines present in selected objects, in order to investigate their correlation with continuum intensity. Preliminary results obtained on
作者: 商品    時間: 2025-3-22 12:01

作者: separate    時間: 2025-3-22 15:11

作者: 憤慨一下    時間: 2025-3-22 20:49
Anisotropic ionising continuum emission in AGNs,N. The anisotropy of the ionising continuum, evident from very extended and very narrow [OIII] line emission, appears correlated with the nuclear radio axis. Further information on anisotropy may be obtained from the detailed associations between [OIII] features and radio components observed in AGNs
作者: Humble    時間: 2025-3-22 22:47

作者: 拾落穗    時間: 2025-3-23 03:43
Polarization OF BL Lac objects, and Faraday rotation. Wavelength- and time-dependent polarization observations of BL Lac itself are used to investigate the polarization characteristics of one variability event without resorting to the use of adjustable fitting parameters. Simultaneous and nearly-simultaneous optical and radio pol
作者: heckle    時間: 2025-3-23 08:41

作者: pulmonary    時間: 2025-3-23 10:23

作者: Anticoagulants    時間: 2025-3-23 16:10

作者: 發(fā)芽    時間: 2025-3-23 20:01
Manganese in Health and Diseasexdensity and polarization for individual core-dominant AGN at . (Wills, Hough, Bailey, Wills and Ballard 1988)—we have discovered steep ( α ?1.8) IRoptical synchrotron components, distinct from the flatter, unpolarized Big Blue Bump (accretion disk?) and 3 pin μm components, in 6 of 18 “normal” quas
作者: palliative-care    時間: 2025-3-23 22:42
VLBI polarization measurements of BL Lacertae objects,
作者: 反抗者    時間: 2025-3-24 03:15
The physical conditions and orientations of parsec-scale jets derived FROM CM-waveband variability
作者: 打擊    時間: 2025-3-24 09:33

作者: 凹處    時間: 2025-3-24 11:50
Optical photometry and polarimetry of BL Lacertae objects,
作者: concubine    時間: 2025-3-24 16:49

作者: hurricane    時間: 2025-3-24 19:16
Narrow band imaging close to the nuclei of BL Lac objects,bserved through a 300 ? wide continuum filter. For comparison, similar observations were made of a Seyfert galaxy and a quasar, both known to exhibit extended gaseous emission..Data reduction is not yet complete but our preliminary results indicate that one of the six BL Lacs we observed displayed e
作者: 洞察力    時間: 2025-3-25 03:07
Optical-infrared synchrotron emission in luminous AGN,xdensity and polarization for individual core-dominant AGN at . (Wills, Hough, Bailey, Wills and Ballard 1988)—we have discovered steep ( α ?1.8) IRoptical synchrotron components, distinct from the flatter, unpolarized Big Blue Bump (accretion disk?) and 3 pin μm components, in 6 of 18 “normal” quas
作者: 獨行者    時間: 2025-3-25 04:35

作者: DEVIL    時間: 2025-3-25 10:47
Handbook of Neuropsychology and AgingWe have measured radio polarization of about 90 blazars at 3cm with the 45-m radio telescope of Nobeyama Radio Observatory. Polarization degree and angle of the blazars exhibit significant correlations with their VLBI structure, and core dominance.The correlations are explained by mixture with the extended polarized flux or aberration effect.
作者: 思想    時間: 2025-3-25 13:54

作者: Mosaic    時間: 2025-3-25 18:52

作者: 音的強弱    時間: 2025-3-25 21:16

作者: Pruritus    時間: 2025-3-26 00:23
https://doi.org/10.1007/978-1-59259-165-7Results of photographic observations of three BL Lac objects: ON 231, ON 325 and RS 4 are presented. Our measurements and previous data were combined to construct light curves extending over the last 20 years. No clear periodic behaviour was found. Some possible correlations of optical data with information available in other bands are discussed.
作者: enormous    時間: 2025-3-26 07:34
Statistical properties of radio polarization of blazars,We have measured radio polarization of about 90 blazars at 3cm with the 45-m radio telescope of Nobeyama Radio Observatory. Polarization degree and angle of the blazars exhibit significant correlations with their VLBI structure, and core dominance.The correlations are explained by mixture with the extended polarized flux or aberration effect.
作者: 鞠躬    時間: 2025-3-26 09:51
Radio variability of BL Lacs and related objects: Observations vs. shocked jet models,The properties of compact extragalactic radio sources are investigated using a sample of 27 sources extensively observed at millimeter frequencies. It is suggested that the radio variability of all AGN, independent of their classification, can be understood in terms of growing and decaying shocks in a jet.
作者: Rodent    時間: 2025-3-26 16:19

作者: Palpable    時間: 2025-3-26 18:52
Simultaneous UBVRI polarimetry of blazars,We present simultaneous UBVRI photopolarimetry of 12 blazars and one low polarization quasar, 3C 273. The aim of our observations has been to study frequency-dependent polarization in these sources.
作者: FAST    時間: 2025-3-27 00:48
Long-term optical variability of BL Lac objects,Results of photographic observations of three BL Lac objects: ON 231, ON 325 and RS 4 are presented. Our measurements and previous data were combined to construct light curves extending over the last 20 years. No clear periodic behaviour was found. Some possible correlations of optical data with information available in other bands are discussed.
作者: 神經    時間: 2025-3-27 04:12
Lecture Notes in Physicshttp://image.papertrans.cn/b/image/180127.jpg
作者: Orgasm    時間: 2025-3-27 07:47
https://doi.org/10.1007/BFb0031137BL Lac object; Gravitation; black hole; gravitational lens; gravity; interstellar matter; relativistic jet
作者: Nonthreatening    時間: 2025-3-27 10:13

作者: In-Situ    時間: 2025-3-27 17:01
Mark R. Lovell,Stanley S. Smithn bright, core-dominated sources, the effect has been found in sources with different morphologies, core strengths, and identifications. The list of superluminals is still dominated by quasars but it now includes several BL Lac objects.
作者: 車床    時間: 2025-3-27 18:44

作者: eulogize    時間: 2025-3-27 23:16

作者: expound    時間: 2025-3-28 04:36
https://doi.org/10.1007/978-3-031-15080-7izable sample of objects through detection of weak spectral features, either in emission or in absorption; .) monitoring intensity and profile of the broad emission fines present in selected objects, in order to investigate their correlation with continuum intensity. Preliminary results obtained on
作者: oracle    時間: 2025-3-28 10:11

作者: 強所    時間: 2025-3-28 11:38

作者: 實現    時間: 2025-3-28 17:00

作者: 飛行員    時間: 2025-3-28 21:27
Manganese in Health and Diseased measurements of a sample of 122 core-dominant radio quasars, including BL Lac objects (Wills, Antonucci, Barvainis, Breger and Wills 1988) show:(.) more than half have a significant synchrotron component, with degree of polarization, ., > 3%, (.) there is a very significant decrease in the fractio
作者: 減至最低    時間: 2025-3-29 01:26

作者: Bernstein-test    時間: 2025-3-29 03:36
Michelle K. Nihei,Tomás R. Guilarteplete, flux limited sample of BL Lacs from B = 16 to 18.5. This will allow various problems including the surface density of BL Lacs to be studied. Our survey uses optical plates obtained with the Palomar 48-inch Schmidt telescope and covers 648 square degrees of the sky. The plates are complete to
作者: VEST    時間: 2025-3-29 07:19

作者: refraction    時間: 2025-3-29 12:22

作者: 牙齒    時間: 2025-3-29 18:32

作者: BARB    時間: 2025-3-29 20:42
Handbook of Neuropsychology and AgingFrom a purely statistical point of view this might be due to their being the low-. tail of the quasar distribution; this also would help to explain the rapid intensity variations and high continuum/line ratios. However this explanation is unlikely, because the redshift distributions are so different.
作者: reflection    時間: 2025-3-30 00:08

作者: Statins    時間: 2025-3-30 04:12
Survey of Selective Neurotoxins. The rate of occurrence of both types of [OIII] emission as well as conceivable clues from the observed orientations are discussed. The [OIII] emission in 3C 120 may provide evidence of relativistic beaming.
作者: 挑剔為人    時間: 2025-3-30 11:15

作者: 杠桿    時間: 2025-3-30 16:04

作者: 公社    時間: 2025-3-30 20:27

作者: Thymus    時間: 2025-3-30 23:09

作者: 感情    時間: 2025-3-31 01:14
Polarization OF BL Lac objects,ics of one variability event without resorting to the use of adjustable fitting parameters. Simultaneous and nearly-simultaneous optical and radio polarization measurements (including those made with VLBI) of Q7 287 are also compared and discussed. A method of parameterizing the variability of polarized sources is outlined.
作者: NEG    時間: 2025-3-31 05:47

作者: 尊敬    時間: 2025-3-31 12:29
Conference proceedings 1989ontinuum emission over the whole electromagnetic system and its variability, and the impact of these observations on gravitational lensing and cosmological evolution. The book should be immensely useful for graduate students.
作者: 不舒服    時間: 2025-3-31 13:33
0075-8450 ter, the continuum emission over the whole electromagnetic system and its variability, and the impact of these observations on gravitational lensing and cosmological evolution. The book should be immensely useful for graduate students.978-3-662-13739-0978-3-540-46203-3Series ISSN 0075-8450 Series E-ISSN 1616-6361
作者: 觀點    時間: 2025-3-31 19:25
https://doi.org/10.1007/978-3-031-15080-7evant to the high redshift (. > 0.6) radio galaxies which show even closer alignments between radio and emission line and optical/UV continuum structures. Potentially, observations of the EELR will allow us to place constraints on properties like the opening angle, power and spectrum of blazar beams.
作者: Charitable    時間: 2025-3-31 23:48

作者: 流逝    時間: 2025-4-1 02:44

作者: 粗魯性質    時間: 2025-4-1 09:28
An optical polarization survey for BL Lacs,te, forty candidates from 72 square degrees of the sky have been followed up spectroscopically. A quasar with a redshift of z = 1.42 was found. We consider it a strong candidate to be a highly polarized quasar. Two candidate BL Lacs, objects with apparently featureless spectra, were also found.
作者: 偏離    時間: 2025-4-1 12:36
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作者: 戰(zhàn)勝    時間: 2025-4-1 18:20
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作者: 錯事    時間: 2025-4-1 18:54
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作者: Popcorn    時間: 2025-4-2 01:52
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作者: 煩擾    時間: 2025-4-2 06:49
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作者: 懲罰    時間: 2025-4-2 10:58
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作者: acolyte    時間: 2025-4-2 14:56
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