STRI
发表于 2025-3-21 18:39:35
书目名称Cosmic Explosions影响因子(影响力)<br> http://impactfactor.cn/2024/if/?ISSN=BK0238877<br><br> <br><br>书目名称Cosmic Explosions影响因子(影响力)学科排名<br> http://impactfactor.cn/2024/ifr/?ISSN=BK0238877<br><br> <br><br>书目名称Cosmic Explosions网络公开度<br> http://impactfactor.cn/2024/at/?ISSN=BK0238877<br><br> <br><br>书目名称Cosmic Explosions网络公开度学科排名<br> http://impactfactor.cn/2024/atr/?ISSN=BK0238877<br><br> <br><br>书目名称Cosmic Explosions被引频次<br> http://impactfactor.cn/2024/tc/?ISSN=BK0238877<br><br> <br><br>书目名称Cosmic Explosions被引频次学科排名<br> http://impactfactor.cn/2024/tcr/?ISSN=BK0238877<br><br> <br><br>书目名称Cosmic Explosions年度引用<br> http://impactfactor.cn/2024/ii/?ISSN=BK0238877<br><br> <br><br>书目名称Cosmic Explosions年度引用学科排名<br> http://impactfactor.cn/2024/iir/?ISSN=BK0238877<br><br> <br><br>书目名称Cosmic Explosions读者反馈<br> http://impactfactor.cn/2024/5y/?ISSN=BK0238877<br><br> <br><br>书目名称Cosmic Explosions读者反馈学科排名<br> http://impactfactor.cn/2024/5yr/?ISSN=BK0238877<br><br> <br><br>
conference
发表于 2025-3-21 21:07:09
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Legend
发表于 2025-3-22 01:01:20
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.
态度暖昧
发表于 2025-3-22 04:56:24
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LAVA
发表于 2025-3-22 09:24:57
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Modify
发表于 2025-3-22 16:00:44
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).
Modify
发表于 2025-3-22 17:51:56
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LUCY
发表于 2025-3-23 01:08:13
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牙齿
发表于 2025-3-23 04:12:20
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.
prosthesis
发表于 2025-3-23 08:51:49
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.