標(biāo)題: Titlebook: ; [打印本頁] 作者: CURD 時(shí)間: 2025-3-21 17:51
書目名稱Groups of Galaxies in the Nearby Universe影響因子(影響力)
書目名稱Groups of Galaxies in the Nearby Universe影響因子(影響力)學(xué)科排名
書目名稱Groups of Galaxies in the Nearby Universe網(wǎng)絡(luò)公開度
書目名稱Groups of Galaxies in the Nearby Universe網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Groups of Galaxies in the Nearby Universe被引頻次
書目名稱Groups of Galaxies in the Nearby Universe被引頻次學(xué)科排名
書目名稱Groups of Galaxies in the Nearby Universe年度引用
書目名稱Groups of Galaxies in the Nearby Universe年度引用學(xué)科排名
書目名稱Groups of Galaxies in the Nearby Universe讀者反饋
書目名稱Groups of Galaxies in the Nearby Universe讀者反饋學(xué)科排名
作者: 遺忘 時(shí)間: 2025-3-21 21:23 作者: 壓倒性勝利 時(shí)間: 2025-3-22 01:52
Physical Examination of the Shoulderusing independent distances we will be able to derive Hi mass functions and local star formation densities for the Local Volume as well as nearby galaxy groups such as the CenA and Sculptor groups. A complementary .-band survey will also allow us to analyse the (baryonic) Tully-Fisher relation.作者: 領(lǐng)袖氣質(zhì) 時(shí)間: 2025-3-22 08:14 作者: 微生物 時(shí)間: 2025-3-22 11:17
Reaction kinetics of coordination compounds,iends of Friends algorithm. It is important to stress, however, that there are also important differences, whose discussion could be useful to gain insight on the nature of galaxy groups, and to complement the results of other studies.作者: 不如屎殼郎 時(shí)間: 2025-3-22 16:56 作者: 不如屎殼郎 時(shí)間: 2025-3-22 18:51 作者: 暫時(shí)中止 時(shí)間: 2025-3-22 22:02 作者: 有斑點(diǎn) 時(shí)間: 2025-3-23 04:57
Properties of RR Lyrae Stars in the Inner Regions of the Large Magellanic Cloud. II. The Extended SaLMC RR Lyrae, and metallicities for 78 RR Lyrae, nearly tripling the previous sample. These targets are located in 11 fields covering a wide range of distances, out to 2.5 degrees from the center of the LMC. The sample allows us to compare the kinematics of the old and metal-poor stars in the LMC with the rest of the stellar populations.作者: BANAL 時(shí)間: 2025-3-23 08:27
Diffuse Ionized Gas in the Dwarf Galaxy DDO 53 galaxies, the spectral characteristics are very diferent to those of the DIG in spiral galaxies: the excitation is higher and the [SII/Hα] much lower. A combination of leakage photoionization models plus shocks will be able to explain these characteristics.作者: 無節(jié)奏 時(shí)間: 2025-3-23 10:51 作者: 馬籠頭 時(shí)間: 2025-3-23 16:28 作者: chemical-peel 時(shí)間: 2025-3-23 18:26
Gravity field outside the earth, galaxies, the spectral characteristics are very diferent to those of the DIG in spiral galaxies: the excitation is higher and the [SII/Hα] much lower. A combination of leakage photoionization models plus shocks will be able to explain these characteristics.作者: 忘川河 時(shí)間: 2025-3-24 00:12 作者: 察覺 時(shí)間: 2025-3-24 02:44
Local Group(s)he M81 group, the CenA group, and the IC 342/Maffei group – are in many respects Local Group analogs: Their luminosity functions, galaxy content, fractional galaxy type distribution, crossing times, masses, and zero-velocity surface radii are similar to those of the Local Group. Also, the nearby gro作者: 吹氣 時(shí)間: 2025-3-24 10:12 作者: 憤慨一下 時(shí)間: 2025-3-24 13:20 作者: 網(wǎng)絡(luò)添麻煩 時(shí)間: 2025-3-24 16:30
Properties of RR Lyrae Stars in the Inner Regions of the Large Magellanic Cloud. II. The Extended Saield and 13 in the clusters NGC1835 and NGC2019. 15 RR Lyrae stars of .Cen were observed as well for comparison. We measured radial velocities for 87 LMC RR Lyrae, and metallicities for 78 RR Lyrae, nearly tripling the previous sample. These targets are located in 11 fields covering a wide range of 作者: Essential 時(shí)間: 2025-3-24 21:27 作者: Prostatism 時(shí)間: 2025-3-25 00:37
10mass clusters and groups, drawn from a new 400 deg. X-ray serendipitous survey of Clusters of Galaxies. The aim is to establish robust determinations of the baryon contents in these low-mass systems, and to determine if there is a baryon deficit compared to CMB observations.作者: 逢迎春日 時(shí)間: 2025-3-25 06:37 作者: 多嘴 時(shí)間: 2025-3-25 08:58
Environmental Effects on Galaxy Evolution Based on the Sloan Digital Sky Surveyrelation, we have found two characteristic environments where galaxy morphologies change dramatically, indicating there exist two different physical mechanisms responsible for the cluster galaxy evolution. We also found an unusual population of galaxies, which have spiral morphology but do not have 作者: Ordeal 時(shí)間: 2025-3-25 12:03
The Low-luminosity Galaxy Population in the NGC 5044 Groupong objects originally classified as early-type dwarfs. Particularly, a significant fraction of bright dwarf “ellipticals” show a distinct bulge+disc structure; we thus re-classify these objects as dwarf lenticulars (dS0).作者: gnarled 時(shí)間: 2025-3-25 16:59 作者: 出汗 時(shí)間: 2025-3-25 21:32 作者: 編輯才信任 時(shí)間: 2025-3-26 00:37
https://doi.org/10.1007/978-94-009-9992-3ope and the Australia Telescope Compact Array to produce a census of all the gas-rich galaxies and potential analogs to the high-velocity clouds (HVCs) within these groups down to M. ≤ 10.M.as a test of models of galaxy formation. We present the HI mass function and halo mass function for these anal作者: 自作多情 時(shí)間: 2025-3-26 05:30
Spectral Lines of Atmospheric Gases,ield and 13 in the clusters NGC1835 and NGC2019. 15 RR Lyrae stars of .Cen were observed as well for comparison. We measured radial velocities for 87 LMC RR Lyrae, and metallicities for 78 RR Lyrae, nearly tripling the previous sample. These targets are located in 11 fields covering a wide range of 作者: Debate 時(shí)間: 2025-3-26 09:00 作者: 有罪 時(shí)間: 2025-3-26 13:27 作者: Infirm 時(shí)間: 2025-3-26 19:32 作者: 過度 時(shí)間: 2025-3-26 22:41
https://doi.org/10.1007/978-981-19-1649-6relation, we have found two characteristic environments where galaxy morphologies change dramatically, indicating there exist two different physical mechanisms responsible for the cluster galaxy evolution. We also found an unusual population of galaxies, which have spiral morphology but do not have 作者: FATAL 時(shí)間: 2025-3-27 03:11 作者: Feckless 時(shí)間: 2025-3-27 06:00 作者: 洞穴 時(shí)間: 2025-3-27 11:27
Physical Infrastructure Developmentmass clusters and groups, drawn from a new 400 deg. X-ray serendipitous survey of Clusters of Galaxies. The aim is to establish robust determinations of the baryon contents in these low-mass systems, and to determine if there is a baryon deficit compared to CMB observations.作者: enmesh 時(shí)間: 2025-3-27 17:38 作者: 一個(gè)姐姐 時(shí)間: 2025-3-27 20:19 作者: 抗體 時(shí)間: 2025-3-27 23:32 作者: Ophthalmologist 時(shí)間: 2025-3-28 04:49
History of the Physical Dimension,I review the differences and similarities between the dwarf irregular and dwarf spheroidal galaxies in the Local Group. New observations are resolving the long-standing problem of the relationship between dwarf elliptical and dwarf irregular galaxies.作者: Carcinoma 時(shí)間: 2025-3-28 09:26 作者: 高歌 時(shí)間: 2025-3-28 14:11 作者: 北極人 時(shí)間: 2025-3-28 17:25
Vee P. Prasher,Matthew P. JanickiIn this contribution I will provide a brief summary of the history of searches for, and surveys of, galaxy groups. This will be split up into two separate parts, searches with and without galaxy redshift measurements. I will conclude with a more detailed look at a recent result from the 2 degree Field Galaxy Redshift Survey (2dFGRS).作者: 懶洋洋 時(shí)間: 2025-3-28 19:16
https://doi.org/10.1007/978-3-030-55366-1We present here the first results from an ongoing spectroscopic survey of candidate compact groups selected in second Digitized Palomar Observatory Sky Survey, DPOSS II. The survey has been carried out at La Silla Observatory and 120 groups out of 261 possible candidates visible from the southern emisphere have been observed.作者: BRAWL 時(shí)間: 2025-3-28 22:54 作者: white-matter 時(shí)間: 2025-3-29 03:34
https://doi.org/10.1007/978-3-319-97313-5We present a photometric search for UCD candidates in the nearby galaxy group NGC 1023 (d=11 Mpc) – the poorest environment searched for UCDs yet –, based on wide field imaging with CFHT.作者: SEMI 時(shí)間: 2025-3-29 09:17 作者: Glucocorticoids 時(shí)間: 2025-3-29 15:27
The Local Group Dwarfs ComparedI review the differences and similarities between the dwarf irregular and dwarf spheroidal galaxies in the Local Group. New observations are resolving the long-standing problem of the relationship between dwarf elliptical and dwarf irregular galaxies.作者: 吸引力 時(shí)間: 2025-3-29 19:08
Stellar Metallicities and Ages in Leo I dSphWe present the first results of a spectroscopic study of Leo I dSph carried out using FORS2 at the ESO VLT, in which we derive metallicities for 78 red giant stars from the equivalent widths of calcium triplet lines.作者: 不能約 時(shí)間: 2025-3-29 22:29 作者: Generic-Drug 時(shí)間: 2025-3-30 01:09
Galaxy Group Searches and SurveysIn this contribution I will provide a brief summary of the history of searches for, and surveys of, galaxy groups. This will be split up into two separate parts, searches with and without galaxy redshift measurements. I will conclude with a more detailed look at a recent result from the 2 degree Field Galaxy Redshift Survey (2dFGRS).作者: CLAIM 時(shí)間: 2025-3-30 05:28 作者: cardiopulmonary 時(shí)間: 2025-3-30 11:10 作者: 哀求 時(shí)間: 2025-3-30 13:11 作者: Tempor 時(shí)間: 2025-3-30 18:17 作者: Meander 時(shí)間: 2025-3-31 00:19
Atta-ur-Rahman,Viqar Uddin Ahmador chronic cough can be challenging. This chapter describes the pathophysiology of sputum production in asthma, the work-up of asthma in the coughing patient, and an approach to refractory cough in the patient previously diagnosed with asthma.作者: micturition 時(shí)間: 2025-3-31 01:16
Agroecosystem Management,t assessment scenarios of production schemes are compared with the tool of optimisation. An innovative topic is the estimation of regionalised optimum management strategies, depending on site properties. The proposed methodology supports the step of decision support in precision farming.作者: 慷慨援助 時(shí)間: 2025-3-31 08:11
1431-1941 rch and to readers interested in inclusive approaches for cooperative change management and the IT implications for IC platforms..978-3-030-52883-6978-3-030-52881-2Series ISSN 1431-1941 Series E-ISSN 2197-716X 作者: Mnemonics 時(shí)間: 2025-3-31 09:11
Maria Winzer MD,Martina Rauner PhD,Lorenz C. Hofbauer MDll — landslide relationships; (2) multi-factor empirical assessment methods; (3) distributed, physically-based models; and (4) real-time warning systems. Each of these methods has certain strengths and weaknesses related to landslide hazard assessment. Of the land use practices that exacerbate lands作者: BATE 時(shí)間: 2025-3-31 16:47 作者: SIT 時(shí)間: 2025-3-31 20:44 作者: 是限制 時(shí)間: 2025-3-31 23:31
,Entsch?digungspflichtige Hauterkrankungen,als sch?digend erwiesen h?tte, die dann nicht berücksichtigt worden w?re. Nachfolgend k?nnen daher, besonders was den Abschnitt b betrifft, nur die für die Praxis wichtigsten Daten wiedergegeben werden.作者: intelligible 時(shí)間: 2025-4-1 02:50
Datenverarbeitung,ch gerne eine Abhandlung, erschienen 1985 in Readers Digest, über die Einführung eines Büroartikels, in dem ich wichtige Stellen geschw?rzt habe. Auf meine Frage, um welchen Artikel es sich handeln k?nnte, ist die Antwort immer eindeutig, n?mlich um den Computer.作者: 終點(diǎn) 時(shí)間: 2025-4-1 09:20
Discovery Sampling and Selection Modelsrklichkeit nicht macht, also ein lyrisches Gebilde in dem Sinne w?rtlich nimmt, da?,Dichtung‘ und,Leben‘, lyrisches Ich und autobiographisches Ich gleichgesetzt werden:. An dem R?mer Ovid (43 v. Chr.— ca. 18 n. Chr.), der sich anscheinend vergeblich gegen diese Verwechslung von,Leben’ und,Dichtung’
