HEM
发表于 2025-3-21 17:28:14
书目名称Microquasars影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0633414<br><br> <br><br>书目名称Microquasars影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0633414<br><br> <br><br>书目名称Microquasars网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0633414<br><br> <br><br>书目名称Microquasars网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0633414<br><br> <br><br>书目名称Microquasars被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0633414<br><br> <br><br>书目名称Microquasars被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0633414<br><br> <br><br>书目名称Microquasars年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0633414<br><br> <br><br>书目名称Microquasars年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0633414<br><br> <br><br>书目名称Microquasars读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0633414<br><br> <br><br>书目名称Microquasars读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0633414<br><br> <br><br>
言外之意
发表于 2025-3-21 20:21:04
https://doi.org/10.1007/978-94-010-0700-9Accretion; Galaxy; Quasar; astrophysics; relativistic jet; star
arboretum
发表于 2025-3-22 02:12:42
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Hormones
发表于 2025-3-22 08:06:55
Observations of GRS 1915+105 from the USA Experiment on ArgosWe present first results from a monitoring campaign of GRS 1915+105 undertaken with the USA X-ray timing experiment on the ARGOS satellite. A variety of behaviour has been observed, ranging from low, steady X-ray emission to rapid quasi-periodic flaring on timescales of approximately 10–120 seconds.
ELUC
发表于 2025-3-22 11:18:55
Identification of the Donor in GRS 1915+105We report on medium-resolution H and K band spectroscopy of GRS 1915+ 105 using the 8m VLT at ESO. We clearly identify absorption bandheads from .CO/.CO. Together with other features we classify the donor as a K-M III star.
明智的人
发表于 2025-3-22 13:36:32
On the Mass-Donating Star in GRS 1915+105Geometric constraints and the lack of eclipses in GRS 1915+105 are used to place limits on the mass of the companion star. We rule out any companion with .. > 19.4.. for a black hole mass of .. ≃ 30..
flavonoids
发表于 2025-3-22 18:09:48
http://reply.papertrans.cn/64/6335/633414/633414_7.png
别炫耀
发表于 2025-3-23 00:53:56
XTE J1550–564: A Superluminal Ejection During the September 1998 OutburstIn 1998 September, the X-ray transient XTE J155072–564 underwent a major outburst in soft and hard X-rays, followed by a radio flare. Australian Long Baseline Array images obtained shortly after the peak in the radio flare showed evolving structure. The components observed have an apparent separation velocity of > 2..
现晕光
发表于 2025-3-23 02:47:02
Optical Behaviour of XTE J1550–564 and XTE J1859+226 from Outburst to QuiescenceWe present here the optical light curves of the Soft X-ray Transients XTE J1550–564 and XTEJ1859+226 from outburst to quiescence
foppish
发表于 2025-3-23 08:00:12
Minioutbursts in XTE J1859+226Photometry of the X-ray transient XTE J1859+226, obtained during outburst, showed at least 3 minioutbursts. During the second one, the source exhibited a 0.3 mag modulation with QPO flaring activity during the minimum.