Zobrazeno 1 - 10
of 17
pro vyhledávání: '"H. L. Malasan"'
Publikováno v:
IOP Conference Series: Earth and Environmental Science. 1047:012003
This research was conducted to 3D model our meteorite collection based on photo-capturing. This meteorite are from Astomulyo, Central Lampung, Indonesia. It entry the earth's atmosphere and was found on January 28, 2021. The chance of object degradat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c1dc10857387e2a8bd2b8dd992eb883d
https://doi.org/10.1088/1755-1315/1047/1/012003
https://doi.org/10.1088/1755-1315/1047/1/012003
Publikováno v:
Journal of Physics: Conference Series. 2214:012007
A planetary nebula is formed when a low to intermediate mass star approaches the end of its life. Before the ejected materials finally interact with and dissipate into the interstellar matters, the nebula will be visible surrounding its former stella
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1e16bf8b1f80fa9bd7d6de1dc69808bd
https://doi.org/10.1088/1742-6596/2214/1/012007
https://doi.org/10.1088/1742-6596/2214/1/012007
Publikováno v:
Journal of Physics: Conference Series. 2214:012012
We report low and intermediate resolution spectra of the recurrent nova RS Oph taken at two observatories. A low resolution spectrum (R ≈ 1000) was taken at ITERA Astronomical Observatory (IAO) in Lampung by using 25 cm (f/8) RC Astrograph telescop
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bcb75ed4b4907ac326baa55ed6b81f74
https://doi.org/10.1088/1742-6596/2214/1/012012
https://doi.org/10.1088/1742-6596/2214/1/012012
Autor:
C Vidante, H L Malasan
Publikováno v:
Journal of Physics: Conference Series. 2214:012005
Eclipsing binary is an edge-on binary system where the components appear to be eclipsing one another. Eclipsing binaries therefore give a lot of information on the systems’ behavior, one of them from their period change. O-C diagram exhibits the de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a4257385f1a78e22de641aaa1d4c943e
https://doi.org/10.1088/1742-6596/2214/1/012005
https://doi.org/10.1088/1742-6596/2214/1/012005
Autor:
D G Harbowo, R Muztaba, H L Malasan, S Sumardi, L K Agustina, T Julian, J H Sitorus, A D A Denhi, D J P Sihombing, M P Mahayu, D Setyawan
Publikováno v:
IOP Conference Series: Earth and Environmental Science. 882:012011
In early 2021, a rare extraterrestrial object passed at high speed, followed by a powerful boom, with a bright flare crossing the atmosphere and falling in Astomulyo Village, Punggur, Central Lampung, Indonesia. This object has been scientifically de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3efd10d1a7e01527d14c4b80df60435f
https://doi.org/10.1088/1755-1315/882/1/012011
https://doi.org/10.1088/1755-1315/882/1/012011
Autor:
Andrea Richichi, G. K. Haans, P. Irawati, R. Azaliah, J. Suherli, B. Soonthornthum, Z. M. Arifin, H. L. Malasan, S. Akhyar, D. G. Ramadhan, T. Sarotsakulchai
Publikováno v:
Publications of The Korean Astronomical Society. 30:205-209
The Eclipsing Binaries Minima (BIMA) Monitoring Project is a CCD-based photometric observational program initiated by Bosscha Observatory - Lembang, Indonesia in June 2012. Since December 2012 the National Astronomical Research Institute of Thailand
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f85b915abd4d2976dce697afe76a7bd8
https://doi.org/10.5303/pkas.2015.30.2.205
https://doi.org/10.5303/pkas.2015.30.2.205
Autor:
R. Darma, H. L. Malasan
Publikováno v:
Journal of Physics: Conference Series. 1245:012008
α Tau is an interesting Red Giant Branch (RGB) star with spectral type K5, yet not well studied. Helium core contraction and hydrogen burning in the shell are occurring in this star. Stars like α Tau are interested to be investigated in order to le
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f4afaf8207c1cddb69ee8239e2a0aca1
https://doi.org/10.1088/1742-6596/1245/1/012008
https://doi.org/10.1088/1742-6596/1245/1/012008
Autor:
E. Puspitaningrum, H. L. Malasan
Publikováno v:
Journal of Physics: Conference Series. 1231:012031
Observations of the central star planetary nebulae (CSPN) IC 4663 revealed its spectral features similar to WN sequence of massive Wolf-Rayet (WR) stars. Because CSPN IC 4663 spectrum is dominated by broad He II and N V emission lines, it is classifi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a5d70a744707d18e013e38ee208e2a28
https://doi.org/10.1088/1742-6596/1231/1/012031
https://doi.org/10.1088/1742-6596/1231/1/012031
Publikováno v:
Journal of Physics: Conference Series; 2019, Vol. 1245 Issue 1, p1-1, 1p
Publikováno v:
Journal of Physics: Conference Series; 2019, Vol. 1231 Issue 1, p1-1, 1p