Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Lipunov, Vladimir M."'
Autor:
Trigg, Aaron C., Burns, Eric, Roberts, Oliver J., Negro, Michela, Svinkin, Dmitry S., Baring, Matthew G., Wadiasingh, Zorawar, Christensen, Nelson L., Andreoni, Igor, Briggs, Michael S., Di Lalla, Niccolo, Frederiks, Dmitry D., Lipunov, Vladimir M., Omodei, Nicola, Ridnaia, Anna V., Veres, Peter, Lysenko, Alexandra L.
Publikováno v:
A&A 687, A173 (2024)
Magnetars are slowly rotating neutron stars that possess the strongest magnetic fields ($10^{14}-10^{15} \mathrm{G}$) known in the cosmos. They display a range of transient high-energy electromagnetic activity. The brightest and most energetic of the
Externí odkaz:
http://arxiv.org/abs/2311.09362
Autor:
Burgess, J. Michael, Greiner, Jochen, Begue, Damien, Giannios, Dimitrios, Berlato, Francesco, Lipunov, Vladimir M.
The recent coincident detection of gravitational waves (GW) from a binary neutron star merger with aLIGO/Virgo and short-lived gamma-ray emission with Fermi/GBM (called GW 170817) is a milestone for the establishment of multi-messenger astronomy. Mer
Externí odkaz:
http://arxiv.org/abs/1710.05823
Autor:
Trigg, Aaron C., Burns, Eric, Roberts, Oliver J., Negro, Michela, Svinkin, Dmitry S., Baring, Matthew G., Wadiasingh, Zorawar, Christensen, Nelson L., Andreoni, Igor, Briggs, Michael S., Di Lalla, Niccolò, Frederiks, Dmitry D., Lipunov, Vladimir M., Omodei, Nicola, Ridnaia, Anna V., Veres, Peter, Lysenko, Alexandra L.
Publikováno v:
Astronomy & Astrophysics / Astronomie et Astrophysique; 7/15/2024, Vol. 687, p1-12, 12p
Autor:
Lipunov, Vladimir M., Gorbovskoy, E., Kornilov, V., Krushinskiy, V., Vlasenko, D., Tiurina, N., Balanutsa, P., Kuznetsov, A., Budnev, N., Gress, O., Tlatov, A., Lopez, R. Rebolo, Serra-Ricart, M., Buckley, D. A. H., Israelian, G., Lodieu, N., Ivanov, K., Yazev, S., Sergienko, Yu., Gabovich, A., Yurkov, V., Levato, H., Saffe, C., Podesta, R., Mallamaci, C., Lopez, C.
On 2015 June 15 the Swift space observatory discovered that the Galactic black hole candidate V404 Cyg was undergoing another active X-ray phase, after 25 years of inactivity (Barthelmy et al. 2015). Twelve telescopes of the MASTER Global Robotic Net
Externí odkaz:
http://arxiv.org/abs/1608.02764
Autor:
Lipunov, Vladimir M.1,2 (AUTHOR) akuznetsov@sai.msu.ru, Kornilov, Viktor G.1,2 (AUTHOR) gorbovskoy@sai.msu.ru, Zhirkov, Kirill1 (AUTHOR) vlasenko@sai.msu.ru, Kuznetsov, Artem2 (AUTHOR) tiurina@sai.msu.ru, Gorbovskoy, Evgenii2 (AUTHOR) gress@sai.msu.ru, Budnev, Nikolai M.3 (AUTHOR) nbudnev@api.isu.ru, Buckley, David A. H.4 (AUTHOR) dah.buckley@saao.nrf.ac.za, Lopez, Rafael Rebolo5 (AUTHOR) rrl@iac.es, Serra-Ricart, Miquel5 (AUTHOR) mserra@iac.es, Francile, Carlos6,7 (AUTHOR) cfrancile@unsj-cuim.edu.ar, Tyurina, Nataly2 (AUTHOR) balanutsa@sai.msu.ru, Gress, Oleg2,3 (AUTHOR) ershova@sai.msu.ru, Balanutsa, Pavel2 (AUTHOR) minkina@sai.msu.ru, Antipov, Gleb2 (AUTHOR) senik@sai.msu.ru, Vlasenko, Daniil1,2 (AUTHOR) topolev@sai.msu.ru, Topolev, Vladislav1,2 (AUTHOR) chasovnikov@sai.msu.ru, Chasovnikov, Aristarkh1,2 (AUTHOR) sis@coronas.ru, Svertilov, Sergei I.1,8 (AUTHOR) kuvshinov@sai.msu.ru, Podesta, Ricardo6,7 (AUTHOR) ricpod@hotmail.com, Podesta, Federico6,7 (AUTHOR) karmaguitar@hotmail.com
Publikováno v:
Universe (2218-1997). May2022, Vol. 8 Issue 5, p271-271. 27p.
Autor:
Lipunov, Vladimir M.
Publikováno v:
Grav.Cosmol. 11 (2005) 166-168
Recently estimation of merger rate of double neutron stars from the observations of PSR J0737-3039 by Burgay is discussed under real astrophysical background.
Comment: 8 pages, including 3 figures. ASS, in press
Comment: 8 pages, including 3 figures. ASS, in press
Externí odkaz:
http://arxiv.org/abs/astro-ph/0406502
Autor:
Lipunov, Vladimir M.
The Invited Review on Joint Discussion "High Energy Transients" on XXIIIrd General Assembly of IAU, Kioto, 1997 is presented. The simulated rates of neutron star + neutron star, neutron star + black hole and black hole + black hole mergings are consi
Externí odkaz:
http://arxiv.org/abs/astro-ph/9711270
Autor:
Lipunov, Vladimir M.
The simulated rates of NS+NS, NS+BH and BH+BH mergings are considered in relation with the problem of GRBursts origin and gravitational waves detection.
Comment: 5 pages, LaTeX, jd.sty, 4 figures
Comment: 5 pages, LaTeX, jd.sty, 4 figures
Externí odkaz:
http://arxiv.org/abs/astro-ph/9711244
Publikováno v:
New Astron. 2 (1997) 555-558
The possible low-frequency radio emission from the progenitors of gamma ray bursts can experience a delay from tens of seconds to hours on the way to the observer due to the dispersion in galactic and extragalactic plasma, and thus reach the observer
Externí odkaz:
http://arxiv.org/abs/astro-ph/9706074
Publikováno v:
Astron.Astrophys.312:937,1996
Binary neutron stars mergers that are expected to be the most powerful source of energy in the Universe definitely exist in nature, as is proven by the observed behavior of the Hulse-Taylor binary radio pulsar. Though most of energy in such events is
Externí odkaz:
http://arxiv.org/abs/astro-ph/9608155