標(biāo)題: Titlebook: Spiral Galaxies in the Near-IR; Proceedings of the E Dante Minniti,Hans-Walter Rix Conference proceedings 1996 Springer-Verlag Berlin Heide [打印本頁] 作者: Interpolate 時(shí)間: 2025-3-21 19:50
書目名稱Spiral Galaxies in the Near-IR影響因子(影響力)
書目名稱Spiral Galaxies in the Near-IR影響因子(影響力)學(xué)科排名
書目名稱Spiral Galaxies in the Near-IR網(wǎng)絡(luò)公開度
書目名稱Spiral Galaxies in the Near-IR網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Spiral Galaxies in the Near-IR被引頻次
書目名稱Spiral Galaxies in the Near-IR被引頻次學(xué)科排名
書目名稱Spiral Galaxies in the Near-IR年度引用
書目名稱Spiral Galaxies in the Near-IR年度引用學(xué)科排名
書目名稱Spiral Galaxies in the Near-IR讀者反饋
書目名稱Spiral Galaxies in the Near-IR讀者反饋學(xué)科排名
作者: Ordeal 時(shí)間: 2025-3-21 20:58 作者: jumble 時(shí)間: 2025-3-22 00:37 作者: 助記 時(shí)間: 2025-3-22 06:18
Bargmann 1977). At each angle of the polygonal formation, portal areas or triangular portal tracts with three characteristic structures — the hepatic artery, the portal vein, and the bile duct — are located. These structures run longitudinally along the edges of the lobule, which has an elongated or作者: Confound 時(shí)間: 2025-3-22 11:26
Donald M. Terndruped by. Criticism is directed equally at "loud- mouthed and incompetent anti-nuclear environmentalists", the "nu- clear Byzantium" of the international nuclear establishment, the "in- tellectual narcissism" of those nuclear experts that dare to admit the importance of societal issues, and the tendenc作者: 尋找 時(shí)間: 2025-3-22 14:01
Roelof S. de Jonged by. Criticism is directed equally at "loud- mouthed and incompetent anti-nuclear environmentalists", the "nu- clear Byzantium" of the international nuclear establishment, the "in- tellectual narcissism" of those nuclear experts that dare to admit the importance of societal issues, and the tendenc作者: 召集 時(shí)間: 2025-3-22 18:02 作者: AGOG 時(shí)間: 2025-3-23 00:08 作者: Costume 時(shí)間: 2025-3-23 01:43 作者: Infelicity 時(shí)間: 2025-3-23 06:18 作者: 蔓藤圖飾 時(shí)間: 2025-3-23 10:01
Patricia Whitelockt communities regarding participatory decision making and compensation and the steps that have been or are being taken to promote dialogue and constructive problem-solving are also considered.?978-3-658-08961-0978-3-658-08962-7Series ISSN 2626-2827 Series E-ISSN 2626-2835 作者: septicemia 時(shí)間: 2025-3-23 15:37
R. Michael Richt communities regarding participatory decision making and compensation and the steps that have been or are being taken to promote dialogue and constructive problem-solving are also considered.?978-3-658-08961-0978-3-658-08962-7Series ISSN 2626-2827 Series E-ISSN 2626-2835 作者: 清洗 時(shí)間: 2025-3-23 18:22 作者: limber 時(shí)間: 2025-3-24 00:57 作者: floaters 時(shí)間: 2025-3-24 05:17
Y. K. Ng,G. Bertelli,C. Chiosi,A. Bressan Concerns about safety and exposures, and associated emotions and feelings were the strongest correlates of support for nuclear technology..In 2010, trust of DOE and other responsible parties averaged about 70 % for federal agencies and contractors. One year later, after Fukushima, trust fell approx作者: 善于 時(shí)間: 2025-3-24 08:39 作者: placebo 時(shí)間: 2025-3-24 12:32
PT. India has so far behaved as such by not committing itself to a nuclear weapons programme. Instead, India remains committed to the 1963 Partial Test Ban Treaty (PTBT), and has expressed support for arms control and disarmament measures on a great many occasions.作者: 模仿 時(shí)間: 2025-3-24 18:15 作者: Innocence 時(shí)間: 2025-3-24 20:52 作者: 裹住 時(shí)間: 2025-3-25 00:28 作者: chiropractor 時(shí)間: 2025-3-25 05:21 作者: 情感脆弱 時(shí)間: 2025-3-25 08:10
Photometric and Spectrophotometric Models in the NIRsed. One is a refined spectral synthesis of starbursts in the . band. Another model aims to predict synthetic spectra (continua and lines) and colors of starbursts and the Hubble Sequence from 220? to 5μm.作者: 內(nèi)閣 時(shí)間: 2025-3-25 13:05 作者: 他姓手中拿著 時(shí)間: 2025-3-25 19:30
The Milky Way in the Near-IR, First Results of DENISrn sky, with a 3. detection limit of 18, 16 and 14, in the I, J and .. bands respectively. The DENIS instrument has been in operation at the 1-meter telescope of the European Southern Observatory at La Silla in Chile, since September 1994, with the J and .. channels, and has already provided data on large areas of the sky.作者: 無能性 時(shí)間: 2025-3-25 19:59 作者: idiopathic 時(shí)間: 2025-3-26 03:15
ESO Astrophysics Symposiahttp://image.papertrans.cn/s/image/874450.jpg作者: 夜晚 時(shí)間: 2025-3-26 04:26
https://doi.org/10.1007/978-3-540-49739-4Accretion; Disk Galaxies; Dynamical Structure of Galaxies; Infrared-Observations; Population; Spiral Gala作者: 無法解釋 時(shí)間: 2025-3-26 08:32
Stellar Libraries: Spectral Features in the Near-InfraredThe stellar libraries available in the range 0.8 to 5 μm are reviewed. The strong features present in this range are discussed in the light of synthetic spectra results compared to observations.作者: pacific 時(shí)間: 2025-3-26 14:52 作者: VEN 時(shí)間: 2025-3-26 18:42
1431-2433 Spiral Galaxies in the Near-IR. This meeting took place at the ESO headquarters in Garching bei Miinchen, Germany. The weather waschanging, with the biergarten closed, but that did not stop 85 people from allover the world from attending the meeting. The three days were intensive, with talks and cof作者: 大量 時(shí)間: 2025-3-26 23:50 作者: EXTOL 時(shí)間: 2025-3-27 02:42 作者: Outmoded 時(shí)間: 2025-3-27 08:09
Stellar Populations of Bulges and Disks: New Insights from Near-IR Coloursept for galaxies with special orientations. In this paper we give some results of one of the first studies of galactic bulges and disks in various optical and near-infrared bands, and its implications for the stellar populations of spirals.作者: 否決 時(shí)間: 2025-3-27 11:27
How Much Do Young Stars Contribute to the K-band Light?galaxies are shown to illustrate the role of different star formation histories. Finally, the contribution of young stars to the infrared light is discussed for very simple models of galactic evolution.作者: Nibble 時(shí)間: 2025-3-27 15:22
The Brightest Stars in the Galactic Bulged-luminosity and period-colour relationships. Figures are given for the maximum bolometric and K luminosity of Miras in the Bulge. The period-colour relations differ in different metallicity environments. Although the same may be true of period-luminosity relations, current evidence is inconclusive on this point.作者: obviate 時(shí)間: 2025-3-27 19:22 作者: 終端 時(shí)間: 2025-3-27 22:20 作者: BACLE 時(shí)間: 2025-3-28 03:11
Imaging of Local Group Bulge Populations in the Near Infrarednumbers of long period Miras, which should in principle be younger objects. There is likely to be a wide range in the ages of bulge populations; we point out the case of M33 where there is almost certainly a large age range in the populations of the central 100 pc.作者: Canvas 時(shí)間: 2025-3-28 08:44 作者: OASIS 時(shí)間: 2025-3-28 14:00
When Do Near-IR Colors Help in Studying Stellar Populations?iescent systems such as globular clusters and E/S0 galaxies. However, the presence of dust and active star formation in Irr/BCD and spiral galaxies can significantly reduce the precision of such constraints. At present, an empirical approach to interpreting near-IR colors is favored over a theoretic作者: 激勵(lì) 時(shí)間: 2025-3-28 16:35
Photometric and Spectrophotometric Models in the NIRsed. One is a refined spectral synthesis of starbursts in the . band. Another model aims to predict synthetic spectra (continua and lines) and colors of starbursts and the Hubble Sequence from 220? to 5μm.作者: 國家明智 時(shí)間: 2025-3-28 19:11 作者: 踉蹌 時(shí)間: 2025-3-29 00:58 作者: 裝飾 時(shí)間: 2025-3-29 05:26
Colour Gradients in the Optical and Near-IRroadband colours are easy to obtain for large samples of objects, making them ideal for statistical studies. In this paper I use the radial distribution of the colours in galaxies, which gives more insight into the local processes driving the global colour differences than integrated colours. Almost作者: 衰弱的心 時(shí)間: 2025-3-29 08:31 作者: 脫水 時(shí)間: 2025-3-29 14:04 作者: Alopecia-Areata 時(shí)間: 2025-3-29 18:13 作者: jagged 時(shí)間: 2025-3-29 23:10 作者: defile 時(shí)間: 2025-3-30 00:52
Imaging of Local Group Bulge Populations in the Near Infrarede from a globular cluster-aged stellar population. Giants with .. < -5 are found in M31, M32, and M33, and the HST imaging strongly supports the idea that ground-based observers are not being confused by blended images of stars. On the other hand, a direct measurement of the age of the Galactic bulg作者: 惰性女人 時(shí)間: 2025-3-30 04:06
Origin of Bulgesart of the spheroid formation process, that includes halo and bulge. In a more recently proposed scenario bulges form late, as a result of the dynamical evolution of a disk that is prone to develop a bar instability. Recent . and . results are reported that may help chosing among these two alternati作者: antidote 時(shí)間: 2025-3-30 11:01
The Milky Way in the Near-IR, First Results of DENISrn sky, with a 3. detection limit of 18, 16 and 14, in the I, J and .. bands respectively. The DENIS instrument has been in operation at the 1-meter telescope of the European Southern Observatory at La Silla in Chile, since September 1994, with the J and .. channels, and has already provided data on作者: 助記 時(shí)間: 2025-3-30 15:28
HST Observations of the Ionizing Star Cluster NGC 595 in the Spiral Galaxy M33, B, V, and UV images of the star cluster NGC 595 using the PC chip of the WFPC-2 camera aboard the HST. Photometric reductions were done using DAOPHOT-2. The U-B vs. B-V color-color diagram was used to determined the reddening of each star. The color-magnitude diagram is consistent with a cluster a作者: 前奏曲 時(shí)間: 2025-3-30 19:30
Discovery of the Galactic Bar Population°.0, 3°.9). A better agreement between the observed and the simulated star counts is obtained through the introduction of the ‘bar’ population, which has an age in the range 8–9 Gyr and a metallicity between 0.005 < Z < 0.030.作者: 匍匐前進(jìn) 時(shí)間: 2025-3-30 21:24 作者: evince 時(shí)間: 2025-3-31 04:28 作者: abject 時(shí)間: 2025-3-31 05:56
substantially our knowledge and understanding of the structure, dynamics, and function of morphologi- cal structures, thereby improving upon a purely descriptive presentation. Thus the limits between the individual disciplines in basic research have become blurred. With the development of suitable m作者: 舊石器時(shí)代 時(shí)間: 2025-3-31 12:49
liver is considered to be the classical morphological or anatomical unit of the organ; the results of these early investigations and Kiernan’s (1833) pioneer work in particular has essentially determined our conception of this structure. Around a vein situated centrally in the cross-section and run作者: debris 時(shí)間: 2025-3-31 17:18
