supported through HLM’s Program Penelitian Pengabdian Masyarakat ITB(P2MI)Astronomy Division,FMIPA ITB grant 2022-2023;Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX13AC07G and by other grants and contracts。
We present optical spectra of 10 Galactic Wolf-Rayet(WR)stars that consist of five WN and five WC stars.The optical observation was conducted using a low-resolution spectrograph NEO-R1000(λ/Δλ~1000)at GAO-ITB RTS(2...
Previous simulations studying winds only focus on the line force due to photons from central active galactic nuclei.What properties of the winds will be when including the re-radiation force due to the scattered and r...
supported by the National SKA program of China(2020SKA0120300);the National Key R&D Program of China(2021YFA0718500);the National Natural Science Foundation of China(grant Nos.11833003,12033001);the China Postdoctoral Science Foundation(No.2023T160410);the Opening Foundation of Xinjiang Key Laboratory(No.2021D04016)。
Black widows(BWs)are millisecond pulsars ablating their companion stars.The out-flowing material from the companion can block the radio emission of the pulsar,resulting in eclipses.In this paper,we construct a model f...
Supported by the National Key Research and Development Program of China(2017YFC1501902);Natural Science Foundation of Shanghai Science and Technology Committee(21ZR1457700)。
Accurate prediction of the convection initiation(CI)in urban areas is still a challenge.A heavy rainfall event,missed by the 9-km regional operational modeling system,occurred in the coastal urban area of the Shanghai...
supported by the China Manned Spaced Project(CMS-CSST-2021-B11);National Natural Science Foundation of China(12073091);Guangdong Basic and Applied Basic Research Foundation(2019A1515011119)。
Fast Blue Optical Transients(FBOTs)are luminous transients with fast evolving(typically t;<12 days)light curve and blue color(usually-0.2>g-r>-0.3)that cannot be explained by a supernova-like explosion.We propose a ra...
support from DST/GITA sponsored by the India-Taiwan collaborative project fund(GITA/DST/TWN/P-76/2017);support from DST/SERB sponsored by the Extra Mural Research project(EMR/2016/003918);supported in part by the Higher Education Dept.of the Govt.of West Bengal,India;support from the ISRO sponsored RESPOND project(ISRO/RES/2/418/17-18)fund.
Galactic transient black hole candidate(BHC)MAXI J1836–194 was discovered on 2011 Aug30,by MAXI/GSC and Swift/BAT.The source activity during this outburst continued for^3 months before entering into the quiescent sta...
We investigate the dynamical behavior of a magnetized,dissipative accretion flow around a rapidly rotating black hole.We solve the magnetohydrodynamic equations and calculate the transonic accretion solutions which ma...
Project supported by the National Natural Science Foundation of China(Grant No.11371117).
This paper considers fluid mixing driven by inflows connected to a circular shallow lake using a numerical framework consisting of a shallow water hydrodynamic model and a passive particle-tracking model.With the flow...
The conservation of the energy flux in turbulent jets that propagate in the interstellar medium (ISM) allows us to deduce the law of motion when an inverse power law decrease of density is considered. The back-reactio...