標題: Titlebook: Cosmic Explosions; On the 10th Annivers Juan-María Marcaide,Kurt W. Weiler Conference proceedings 20051st edition Springer-Verlag Berlin He [打印本頁] 作者: STRI 時間: 2025-3-21 18:39
書目名稱Cosmic Explosions影響因子(影響力)
書目名稱Cosmic Explosions影響因子(影響力)學科排名
書目名稱Cosmic Explosions網(wǎng)絡公開度
書目名稱Cosmic Explosions網(wǎng)絡公開度學科排名
書目名稱Cosmic Explosions被引頻次
書目名稱Cosmic Explosions被引頻次學科排名
書目名稱Cosmic Explosions年度引用
書目名稱Cosmic Explosions年度引用學科排名
書目名稱Cosmic Explosions讀者反饋
書目名稱Cosmic Explosions讀者反饋學科排名
作者: conference 時間: 2025-3-21 21:07 作者: Legend 時間: 2025-3-22 01:01
Low Frequency Radio and X-ray Properties of Core-Collapse Supernovaeh (GRB030329) obtained with combined GMRT and VLA data. We report on the low frequency radio monitoring of SN 1995N and our objectives of distinguishing between competing models of X-ray emission from this SN and the nature of its progenitor by X-ray spectroscopy. Radio studies on SN 2001gd, SN 2001ig and SN 2002hh are mentioned.作者: 態(tài)度暖昧 時間: 2025-3-22 04:56 作者: LAVA 時間: 2025-3-22 09:24 作者: Modify 時間: 2025-3-22 16:00
Torture: The Catastrophe of a Bond modeled with two different slopes. The swept-up mass estimate at an age of 3159 days (～0.4 M.), comparable to the low-mass envelope, favors a binary scenario. The observed spectral index of SN 1993J has slowly flattened since age 1000 days onward (α has changed from ?1 to ?0.67 at an age of 2820 days).作者: Modify 時間: 2025-3-22 17:51 作者: LUCY 時間: 2025-3-23 01:08 作者: 牙齒 時間: 2025-3-23 04:12
Translating Trauma, Witnessing Survivale fully-developed dataset, and compare this to our earlier characterization made in 1994. SN 1993J has also been a target of X-ray satellites, and we briefly discuss the nature of the X-ray emission and, together with the radio emission, describe the implications for the nature of the SN’s progenitor.作者: prosthesis 時間: 2025-3-23 08:51
Torture: The Catastrophe of a Bond of SN 1993J further away from us is strongly or totally absorbed. We describe the GFD method and present our findings about the emission structure of the shell. We also present the expansion of SN 1993J based on a method complementary to GFD, which will be described elsewhere.作者: insert 時間: 2025-3-23 10:20 作者: 木訥 時間: 2025-3-23 17:21 作者: 本土 時間: 2025-3-23 21:41
Conservation and Efficiency Issues, to 2002 and show our result on moderately to strongly decelerated expansion with . = 0.71 ± 0.11. We comment on our result of an inversion of the radio spectrum in terms of the emergence of a possible pulsar nebula.作者: subordinate 時間: 2025-3-23 22:41
Conservation and Efficiency Issues,ount of relativistic ejecta, it produces a radio luminosity which is comparable to that seen in the unusual SN1998bw. Using SN2003L as an example, we comment briefly on the broad diversity of type Ic properties and the associated implications for progenitor models.作者: GRAZE 時間: 2025-3-24 02:30
A Decade of Radio and X-ray Observations of SN 1993Je fully-developed dataset, and compare this to our earlier characterization made in 1994. SN 1993J has also been a target of X-ray satellites, and we briefly discuss the nature of the X-ray emission and, together with the radio emission, describe the implications for the nature of the SN’s progenitor.作者: SKIFF 時間: 2025-3-24 09:04 作者: Interlocking 時間: 2025-3-24 11:16
Optical, Ultraviolet, and Infrared Observations of SN 1993Jmission comes from the collision of supernova ejecta with circumstellar gas that was released by the progenitor prior to the explosion. The circumstellar material shows strong evidence of CNO processing.作者: VEST 時間: 2025-3-24 15:36 作者: 貝雷帽 時間: 2025-3-24 21:04 作者: 攤位 時間: 2025-3-25 02:30 作者: 使聲音降低 時間: 2025-3-25 03:41 作者: Exuberance 時間: 2025-3-25 09:51 作者: FLACK 時間: 2025-3-25 12:03 作者: 江湖騙子 時間: 2025-3-25 19:44 作者: exhibit 時間: 2025-3-25 22:32 作者: 字謎游戲 時間: 2025-3-26 03:11
Conservation and Efficiency Issues,h (GRB030329) obtained with combined GMRT and VLA data. We report on the low frequency radio monitoring of SN 1995N and our objectives of distinguishing between competing models of X-ray emission from this SN and the nature of its progenitor by X-ray spectroscopy. Radio studies on SN 2001gd, SN 2001ig and SN 2002hh are mentioned.作者: Water-Brash 時間: 2025-3-26 06:44
Conference proceedings 20051st editionGRB 030329/SN 2003dh, tied the study of SNe and GRBs inextricably together. With the many developments since the last - jor supernova meeting in La Serena, Chile in 1997, we felt that it was an appropriate time to bring together experts and students interested in the subject for a meeting where SN a作者: 辯論 時間: 2025-3-26 09:36 作者: 戰(zhàn)勝 時間: 2025-3-26 15:26
Conservation and Efficiency Issues,, τT ≥ 2.5 during first month, its density (. ～ 10. cm.) and radial extent, ～ (4–5)×10. cm. The plateau-like SN light curve, which we reproduce by a hydrodynamical model, is powered by a combination of internal energy leakage after the explosion of an extended presupernova (～ 10. cm) and subsequent 作者: CLAIM 時間: 2025-3-26 18:25
SN 1994W: Evidence of Explosive Mass Ejection a Few Years Before Explosion, τT ≥ 2.5 during first month, its density (. ～ 10. cm.) and radial extent, ～ (4–5)×10. cm. The plateau-like SN light curve, which we reproduce by a hydrodynamical model, is powered by a combination of internal energy leakage after the explosion of an extended presupernova (～ 10. cm) and subsequent 作者: 愚笨 時間: 2025-3-26 23:36 作者: chastise 時間: 2025-3-27 03:28 作者: 一夫一妻制 時間: 2025-3-27 06:08 作者: 舉止粗野的人 時間: 2025-3-27 13:15
Optical, Ultraviolet, and Infrared Observations of SN 1993Jlentiful. Some results from theoretical modeling of the observations are also discussed. SN 1993J has provided the best observational evidence for the transformation of a SN from one spectral type to another, thereby providing a link between Type II and Type Ib supernovae (SNe). This has strengthene作者: blithe 時間: 2025-3-27 17:41 作者: 出血 時間: 2025-3-27 20:58 作者: 向外供接觸 時間: 2025-3-28 00:06 作者: 強壯 時間: 2025-3-28 04:07
Detection of the Binary Companion to the Progenitor of SN 1993Jomponent in the spectra of SN1993J which cannot be explained by the surrounding faint blue stars. This is the first detection of the expected massive binary companion to the red supergiant progenitor and confirms that SN1993J did indeed arise in an interacting binary system.作者: Infantry 時間: 2025-3-28 08:40 作者: BUCK 時間: 2025-3-28 13:58
VLBI Observations of SN 1979C and SN 1986Jto 22 yr after the explosion, SN 1979C expands .., almost freely, with . = 0.95 ± 0.03. For a total kinetic energy of 3 × 1051 erg, the expansion result requires a mass-loss to wind-velocity ratio for the progenitor of only 1 × 10. M. yr.per 10 km s., an order of magnitude smaller than estimated fro作者: 簡略 時間: 2025-3-28 14:40
SN 1994W: Evidence of Explosive Mass Ejection a Few Years Before Explosionofiles are composed of three major components: (i) narrow P Cygni lines with absorption minima at ?700 km s.; (ii) broad emission lines with blue velocity at zero intensity ～ 4000 km s.; (iii) broad, smooth, extended wings most apparent in H.. These components are identified with the expanding circu作者: 考博 時間: 2025-3-28 20:33 作者: 不妥協(xié) 時間: 2025-3-29 00:13 作者: Osmosis 時間: 2025-3-29 03:10
Synthetic Spectra of the Type Ia SN 2002bois one of the earliest observed SNe. An almost complete set of spectra and photometry is available from 13 days before maximum . light until a few days after. An analysis using synthetic spectra is presented, focusing on the controversial issue of the reddening of SN 2002bo.作者: 無能力之人 時間: 2025-3-29 09:27 作者: Intractable 時間: 2025-3-29 14:34 作者: 粗魯?shù)娜?nbsp; 時間: 2025-3-29 18:11
https://doi.org/10.1007/b137830Cosmology; Redshift; Universe; gamma-ray bursts; stellar candles; supernovae作者: 直覺沒有 時間: 2025-3-29 21:38
978-3-642-42187-7Springer-Verlag Berlin Heidelberg 2005作者: Pulmonary-Veins 時間: 2025-3-30 02:38
Detection of the Binary Companion to the Progenitor of SN 1993Jomponent in the spectra of SN1993J which cannot be explained by the surrounding faint blue stars. This is the first detection of the expected massive binary companion to the red supergiant progenitor and confirms that SN1993J did indeed arise in an interacting binary system.作者: Kinetic 時間: 2025-3-30 07:51 作者: Ophthalmoscope 時間: 2025-3-30 12:08
Radio Supernovaectured circumstellar medium (CSM) and modeling of the radio light curves allows estimation of the physical conditions in this medium. CSM structures, properties of the presupernova system, and the evolution of the system in the last stages before explosion can then be derived.作者: RALES 時間: 2025-3-30 12:46
Torture: The Catastrophe of a BondWe present a selection of our VLBI images of SN 1993J, along with our latest results on its expansion and its shell structure.作者: 侵略者 時間: 2025-3-30 20:35
Translating Trauma, Witnessing SurvivalI describe and interpret observations of the rapidly developing impact of the debris of SN1987A with its circumstellar ring.作者: 推崇 時間: 2025-3-30 22:03
The a-Number of Hyperelliptic Curves,The high resolution obtained through the use of VLBI gives an unique opportunity to directly observe the interaction of an expanding radio supernova with its surrounding medium. We present here results from our VLBI observations of the young supernovae SN 1979C, SN 1986J, and SN 2001gd.作者: 有罪 時間: 2025-3-31 03:53
Nine Years of VLBI Imaging of Supernova 1993JWe present a selection of our VLBI images of SN 1993J, along with our latest results on its expansion and its shell structure.作者: Somber 時間: 2025-3-31 05:12
Supernova 1987A: The Birth of a Supernova RemnantI describe and interpret observations of the rapidly developing impact of the debris of SN1987A with its circumstellar ring.作者: Debility 時間: 2025-3-31 10:40 作者: 主講人 時間: 2025-3-31 16:05
Juan-María Marcaide,Kurt W. WeilerIncludes supplementary material: 作者: 名字的誤用 時間: 2025-3-31 21:34
http://image.papertrans.cn/c/image/238877.jpg作者: 智力高 時間: 2025-3-31 21:44
Translating Trauma, Witnessing Survivalonly a few days after explosion, by our group with the Very Large Array at a number of radio frequencies, as well as by other groups. As a result, it is among the best-studied radio supernovae. The observed synchrotron radio emission is thought to arise from the interaction of the SN shock with the 作者: 闡釋 時間: 2025-4-1 03:26
Torture: The Catastrophe of a Bond circular symmetry. SN 1993J expands according to models of shock excited emission. The angular expansion has a changing deceleration rate and is best modeled with two different slopes. The swept-up mass estimate at an age of 3159 days (～0.4 M.), comparable to the low-mass envelope, favors a binary 作者: tinnitus 時間: 2025-4-1 07:32 作者: 無價值 時間: 2025-4-1 11:24
Translating Trauma, Witnessing Survivallentiful. Some results from theoretical modeling of the observations are also discussed. SN 1993J has provided the best observational evidence for the transformation of a SN from one spectral type to another, thereby providing a link between Type II and Type Ib supernovae (SNe). This has strengthene作者: Ophthalmoscope 時間: 2025-4-1 16:50 作者: 簡略 時間: 2025-4-1 19:24 作者: glacial 時間: 2025-4-1 23:50
