派博傳思國際中心

標(biāo)題: Titlebook: New Quests in Stellar Astrophysics II; Ultraviolet Properti Miguel‘Chavez Dagostino Conference proceedings 2009 The Editor(s) (if applicabl [打印本頁]

作者: Jefferson 時間: 2025-3-21 16:59
書目名稱New Quests in Stellar Astrophysics II影響因子(影響力)

書目名稱New Quests in Stellar Astrophysics II影響因子(影響力)學(xué)科排名

書目名稱New Quests in Stellar Astrophysics II網(wǎng)絡(luò)公開度

書目名稱New Quests in Stellar Astrophysics II網(wǎng)絡(luò)公開度學(xué)科排名

書目名稱New Quests in Stellar Astrophysics II被引頻次

書目名稱New Quests in Stellar Astrophysics II被引頻次學(xué)科排名

書目名稱New Quests in Stellar Astrophysics II年度引用

書目名稱New Quests in Stellar Astrophysics II年度引用學(xué)科排名

書目名稱New Quests in Stellar Astrophysics II讀者反饋

書目名稱New Quests in Stellar Astrophysics II讀者反饋學(xué)科排名

作者: 愛得痛了 時間: 2025-3-21 20:38

作者: Type-1-Diabetes 時間: 2025-3-22 00:28
New Quests in Stellar Astrophysics II978-0-387-87621-4Series ISSN 1570-6591 Series E-ISSN 1570-6605

作者: Inculcate 時間: 2025-3-22 05:23
Miguel‘Chavez DagostinoIncludes supplementary material:

作者: jaunty 時間: 2025-3-22 12:18
GALEX UV Spectroscopy of Extended Objects: The Case of NGC3079,We present UV spectra of the edge-on galaxy NGC3079 obtained with the GALEX slitless grism. We fitted the observed spectra with a young stellar component, various amount of extinction, and several extinction curves. Based on our result, we discuss the use of different extinction curves in order to correct the observed UV fluxes.

作者: intricacy 時間: 2025-3-22 16:46

作者: 粗糙 時間: 2025-3-22 20:11
Astrophysics and Space Science Proceedingshttp://image.papertrans.cn/n/image/665703.jpg

作者: MAIZE 時間: 2025-3-23 01:08

作者: Calculus 時間: 2025-3-23 05:22
,Stellar Populations in Field Early–Type Galaxies,se environments. In particular, luminosity-weighted ages as young as few Gyrs are derived for some galaxies of the sample in the lowest density environments. We suggest that these objects are old galaxies that experienced secondary “rejuvenating” episodes of star formation. We discuss how we will co

作者: 熄滅 時間: 2025-3-23 07:28

作者: 耕種 時間: 2025-3-23 12:13
Conference proceedings 2009only one dedicated to the properties of evolved stellar populations at these wavelengths. This contemporary panorama will be an invaluable resource in the preparation of the next planned space missions, such as the World Space Observatory and the Ultraviolet Imaging Telescope..

作者: 坦白 時間: 2025-3-23 15:40

作者: 怪物 時間: 2025-3-23 18:50
Sperello di Serego Alighieri,Alessandro Bressanewirkt z.B. die Freisetzung der Corticosteroide aus der Nebennierenrinde (Abb. 53) oder das thyreotrope Hormon die Sekretion des Thyroxins aus der Schilddrüse. Andererseits wird durch den Hormonspiegel im Blut die Aktivit?t der Hypophyse und des Zwischenhirns reguliert (Abb. 53).

作者: 法律 時間: 2025-3-24 02:09
Bum-Suk Yeom,Young Kwang Kim,Soo-Chang Rey,Young Hoon Joe,Armando Gil de Pazewirkt z.B. die Freisetzung der Corticosteroide aus der Nebennierenrinde (Abb. 53) oder das thyreotrope Hormon die Sekretion des Thyroxins aus der Schilddrüse. Andererseits wird durch den Hormonspiegel im Blut die Aktivit?t der Hypophyse und des Zwischenhirns reguliert (Abb. 53).

作者: Agronomy 時間: 2025-3-24 06:11

作者: STAT 時間: 2025-3-24 07:44
Rosa A. González-Lópezlira,Alberto Buzzoni et al. 1957, . et al. 1957, . 1958 u.a.) oder chronischer Ganzk?rperbestrahlung (. et al. 1954, . und . 1958) h?ngt stark vom untersuchten . ab. M?usest?mme mit geringerer natürlicher Lebenserwartung ertragen im allgemeinen den Strahleninsult schlechter als solche, die normalerweise ein hohes Alter

作者: 沐浴 時間: 2025-3-24 10:58
Zhanwen Han,Philipp Podsiadlowski,Anthony E. Lynas-Grayosis abnimmt. Man hat schon früh versucht, diese drei Abschnitte mit der Reaktion bestimmter Organsysteme auf die Bestrahlung in Verbindung zu bringen, und in der Tat haben Versuche diese Vermutung best?tigt. Im Bereich A führen die Sch?den des blutbildenden Systems zum Tode (h?matopoetischer Tod),

作者: pantomime 時間: 2025-3-24 18:32

作者: 受人支配 時間: 2025-3-24 19:17
Chang H. Ree,Young-Wook Lee,Sukyoung Yi,Suk-Jin Yoon,GALEX Science Teamtween formal description of dose-effect relations for practical purposes and the mathematical analysis which aims at an understanding of the mechanisms of radiation action. Attention will mainly be given to the dose dependence of cellular radiation actions but the focus will be on general principles

作者: 花束 時間: 2025-3-25 00:30

作者: 閃光你我 時間: 2025-3-25 04:09

作者: ENACT 時間: 2025-3-25 10:53
S. N. Kemp,V. Guzmán Jiménez,P. Ramírez Beraud,J.A. Pérez Grana,V.H. Ramírez Siordia,F.J. Hernández ngen kurz erw?hnt oder aber als unliebsame Komplikationen der experimentellen Sachlage empfunden. Die Zeit war noch nicht reif für ein tieferes Eingehen auf strahlenchemische Erscheinungen, besonders auch, weil eine sachgerechte Molekulartheorie der Materie fehlte. Erst die von . und . begründeten E

作者: 誹謗 時間: 2025-3-25 13:07
I. Puerari,R. A. González–Lópezlira,M. Valdez–Gutiérrezd R?ntgenbildverst?rker-Fernsehsysteme bestimmt. Die Einfallsdosis bzw. Einfallsdosisleistung werden jedoch durch diese beiden apparativ vorgegebenen Gr??en nicht eindeutig festgelegt, obwohl gerade die Einfallsdosen zum Absch?tzen der Strahlenbelastung besonders gut geeignet sind.

作者: Infirm 時間: 2025-3-25 18:40

作者: Sleep-Paralysis 時間: 2025-3-25 22:36

作者: pessimism 時間: 2025-3-26 01:48

作者: RAFF 時間: 2025-3-26 06:21

作者: 伴隨而來 時間: 2025-3-26 10:51

作者: Atmosphere 時間: 2025-3-26 14:53

作者: optional 時間: 2025-3-26 18:46

作者: medieval 時間: 2025-3-27 00:51

作者: Crayon 時間: 2025-3-27 02:37

作者: 人類的發(fā)源 時間: 2025-3-27 08:01
Near-UV Merger Signatures in Early-Type Galaxies,ly-type galaxies without obvious dust or active galactic nuclei. Near-UV imaging is a sensitive probe for the detection of younger components with ages in the range of 10 Myr to 5 Gyr. Only two galaxies have central colors (r< 0.75 r.) that are consistent with a single-generation population. The other ten require a composite population.

作者: 思想靈活 時間: 2025-3-27 12:46
The Impact of Encounters on the Members of Local Group Analogs. A View from , ,axy morphology. UV-bright regions, sites of intense star formation activity accompanied by intense dust extinction, mark the galaxy outskirts forming irregular structures and tails. Compared to the Local Group, LGG 225 seems thus to be experiencing a more intense and active evolutionary phase.

作者: 路標(biāo) 時間: 2025-3-27 15:51
An Atlas of GALEX UV Spectra Selected from the CDFS,d 0.3. The extracted spectra were compared with theoretical templates obtained from the Starburst99 population synthesis code. Two curves of extinction were applied to them in order to estimate the extinction of the selected galaxies.

作者: 無底 時間: 2025-3-27 18:45

作者: 江湖騙子 時間: 2025-3-28 01:57

作者: 星球的光亮度 時間: 2025-3-28 04:06
Colours of the Envelopes of cD Galaxies,ctive star formation. In two cDs with multiple nuclei (A193 and A2634), no colour gradients or regions of current active star formation were found. These results favour an early, ‘primordial origin’ for the cD envelope, the stellar populations of the envelope being coeval with those of the central elliptical galaxy.

作者: 減至最低 時間: 2025-3-28 08:56
A Morphological Study of M81: Comparison Between GALEX and Spitzer Imaging,the origin of UV, 5.8, and 8.0 μm infrared light, and it is an important result pointing in the direction that 5.8 and 8.0 μm light comes from dust illuminated by ultraviolet photons from the very young population.

作者: Esophagitis 時間: 2025-3-28 11:22

作者: 廢除 時間: 2025-3-28 18:31

作者: 形容詞詞尾 時間: 2025-3-28 18:55

作者: Jocose 時間: 2025-3-29 02:53

作者: 暗諷 時間: 2025-3-29 03:15

作者: 使更活躍 時間: 2025-3-29 07:37
The Chemical Composition of Elliptical Galaxies Through Mid-UV Indices,ide. On the basis of the Index vs [Fe/H] correlations seen in a sample of galactic globular clusters, we derived the chemical composition for all our sample galaxies. All resulting abundances are subsolar with Mg features delivering, on average, the lowest values.

作者: 小畫像 時間: 2025-3-29 11:54
The Rest-Frame UV Spectrum of Elliptical Galaxies at High Redshift,a characteristic structure due to a set of iron and magnesium lines lines at λ?eq 2600–2850 ? in the rest frame. The same feature permits also to estimate the time elapsed since the cessation of star formation. Current efforts at observing high redshift PEGs at the VLT and SUBARU telescopes are brie

作者: 過去分詞 時間: 2025-3-29 16:06
Rest-Frame UV and Visible Properties of Early Type Galaxies at 1 < , < 2,vely evolving systems provide constraints on the formation redshift and abundances for the oldest stars at a time when the universe was roughly 1/3 its present age. The passive galaxies have spectra characteristic of F stars with strong absorption from MgII, MgI and FeII. Best fitting ages are in th

作者: Incommensurate 時間: 2025-3-29 21:56

作者: pessimism 時間: 2025-3-30 01:21
,Near UV Properties of Early–Type Galaxies at z ~ 1,ype Galaxies (ETG) at 0.88 作者: 人充滿活力 時間: 2025-3-30 07:36

作者: hauteur 時間: 2025-3-30 09:45

作者: 描述 時間: 2025-3-30 14:34
UV Excess and AGB Evolution in Elliptical-Galaxy Stellar Populations, contributors to galaxy ultraviolet luminosity excess. While a blue HB morphology seems a natural characteristic of metal-poor stellar populations, its appearance in metal-rich systems, often coupled with a poorer rate of planetary nebulae per unit galaxy luminosity, might be calling for an intimate

作者: ear-canal 時間: 2025-3-30 17:21
Binary Stars as the Source of the Far-UV Excess in Elliptical Galaxies,at this UV excess is caused by an old population of hot helium-burning stars without large hydrogen-rich envelopes rather than young stars, their origin has remained a mystery. Here we show that these stars most likely lost their envelopes because of binary interactions, similar to the hot subdwarf

作者: Mystic 時間: 2025-3-31 00:24
,Stellar Populations in Field Early–Type Galaxies,tudy from ultraviolet (UV) to infrared (IR) of a sample 65 nearby ETGs. We derived Lick line-strength indices at different galacto-centric distances from the optical spectra (3700-7000 ?), and extracted ages, metallicites and element abundance ratios for the galaxies by comparison of the indices wit

作者: resuscitation 時間: 2025-3-31 03:35

作者: 錢財 時間: 2025-3-31 07:34

作者: 大喘氣 時間: 2025-3-31 10:51

作者: 無王時期, 時間: 2025-3-31 16:23

作者: LINE 時間: 2025-3-31 20:09

作者: correspondent 時間: 2025-3-31 21:49

作者: 盡忠 時間: 2025-4-1 05:09
An Atlas of GALEX UV Spectra Selected from the CDFS, redshifts were obtained from the Classifying Objects Medium-Band Observations (COMBO) and the selected sample covers a redshift range between 0.02 and 0.3. The extracted spectra were compared with theoretical templates obtained from the Starburst99 population synthesis code. Two curves of extinctio

作者: 最小 時間: 2025-4-1 09:42

作者: Mundane 時間: 2025-4-1 14:00
uch die Arbeitsbedingungen in Joachimsthal, wo er als Stadtarzt t?tig war: ?Der Staub bringt die Lungen zum Eitern und erzeugt im K?rper die Schwindsucht. Auf den Gruben findet man Frauen, die sieben M?nner gehabt haben, welche alle jene unheilvolle Schwindsucht dahingerafft hat.“?Bergsucht” wurde d

作者: gospel 時間: 2025-4-1 14:32
Sperello di Serego Alighieri,Alessandro Bressann verstanden, die von spezialisierten Drüsen (innersekretorischen Drüsen) oder Geweben gebildet, in die Blutbahn sezerniert werden und an den peripheren Erfolgsorganen spezifische Wirkungen entfalten. Man unterscheidet auf Grund ihres chemischen Aufbaus Proteohormone, die aus peptidartig verknüpften

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