Zobrazeno 1 - 10
of 886
pro vyhledávání: '"Richmond, Michael"'
Autor:
Muraoka, Katsuki, Kojiguchi, Naoto, Ito, Junpei, Nogami, Daisaku, Kato, Taichi, Tampo, Yusuke, Taguchi, Kenta, Isogai, Keisuke, Arranz, Teofilo, Blackwell, John, Blane, David, Brincat, Stephen M., Coates, Graeme, Cooney, Walter, Dvorak, Shawn, Galdies, Charles, Glomski, Daniel, Hambsch, Franz-Josef, Harris, Barbara, Hodge, John, Hernández-Verdejo, Jose L., Iozzi, Marco, Itoh, Hiroshi, Kiyota, Seiichiro, Lee, Darrell, Larsson, Magnus, Lahtinen, Tapio, Myers, Gordon, Monard, Berto, Aimar, Mario Morales, Moriyama, Masayuki, Mizutani, Masanori, Nagai, Kazuo, AlQaissieh, Thabet, Gabuya, Aldrin B., Odeh, Mohammad, Perello, Carlos, Pearce, Andrew, Perales, Juan Miguel, Quiles, David, Romanov, Filipp D., Lane, David J., Richmond, Michael, Ruocco, Nello, Sano, Yasuo, Spearman, Mark, Schmidt, Richard, Vanmunster, Tonny, Dubovsky, Pavol A., Wagner, Richard, Wollenhaupt, Guido, Lorenz, Joachim, Lehmann, Gerhard, Salewski, Andrea, Williamson, Guy
We present our optical photometric observations of the 2022 eruption of the recurrent nova U Scorpii (U Sco) using 49,152 data points over 70 d following the optical peak. We have also analyzed its soft X-ray (0.3--1 keV) light curve by the Neil Gehr
Externí odkaz:
http://arxiv.org/abs/2402.06347
Autor:
Tampo, Yusuke, Kato, Taichi, Kojiguchi, Naoto, Shugarov, Sergey Yu., Itoh, Hiroshi, Matsumoto, Katsura, Nakagawa, Momoka, Nishida, Yukitaka, Richmond, Michael, Shibata, Masaaki, Ito, Junpei, Kokhirova, Gulchehra, Rakhmatullaeva, Firuza, Tordai, Tamás, Kiyota, Seiichiro, Ruiz, Javier, Dubovsky, Pavol A., Medulka, Tomáš, Pavlenko, Elena P., Antonyuk, Oksana I., Sosnovskij, Aleksei A., Baklanov, Aleksei V., Krushevska, Viktoriia, Vanmunster, Tonny, Brincat, Stephen M., Petrik, Karol, Galdies, Charles, Hambsch, Franz-Josef, Maeda, Yutaka, Nogami, Daisaku
Superoutbursts in WZ Sge-type dwarf novae (DNe) are characterized by both early superhumps and ordinary superhumps originating from the 2:1 and 3:1 resonances, respectively. However, some WZ Sge-type DNe show a superoutburst lacking early superhumps;
Externí odkaz:
http://arxiv.org/abs/2303.17960
Autor:
Patterson, Joseph, Epstein-Martin, Marguerite, Enenstein, Josie, Kemp, Jonathan, Sabo, Richard, Cooney, Walt, Vanmunster, Tonny, Dubovsky, Pavol, Hambsch, Franz-Josef, Myers, Gordon, Lemay, Damien, Sokolovsky, Kirill, Collins, Donald, Campbell, Tut, Roberts, George, Richmond, Michael, Brincat, Stephen, Ulowetz, Joseph, Dvorak, Shawn, Tordai, Tamas, Dufoer, Sjoerd, Cahaly, Andrew, Galdies, Charles, Goff, Bill, Wilkin, Francis, de Miguel, Enrique, Wood, Matt
We present time-series photometry during eruption of the extremely fast nova V1674 Herculis (Nova Her 2021). The 2021 light curve showed periodic signals at 0.152921(3) d and 501.486(5) s, which we interpret as respectively the orbital and white dwar
Externí odkaz:
http://arxiv.org/abs/2207.00181
Autor:
Hossain, Md Kamal, Haukka, Matti, Lisensky, George C., Richmond, Michael G., Nordlander, Ebbe
Publikováno v:
In Polyhedron 1 August 2024 258
Autor:
Niijima, Keito, Kimura, Mariko, Wakamatsu, Yasuyuki, Kato, Taichi, Nogami, Daisaku, Isogai, Keisuke, Kojiguchi, Naoto, Ohnishi, Ryuhei, Shidatsu, Megumi, Stone, Geoffrey, Hambsch, Franz-Josef, Tordai, Tamás, Richmond, Michael, Vanmunster, Tonny, Myers, Gordon, Brincat, Stephen M., Dubovsky, Pavol A., Medulka, Tomas, Kudzej, Igor, Parimucha, Stefan, Littlefield, Colin, Monard, Berto, Ulowetz, Joseph, Pavlenko, Elena P., Antonyuk, Oksana I., Sosnovskij, Aleksei A., Baklanov, Aleksei V., Antoniuk, Kirill A., Pit, Nikolai V., Belan, Sergei P., Babina, Julia V., Sklyanov, Aleksandr S., Zaostrozhnykh, Anna M., Simon, Andrew V., Cook, Lewis M., Miller, Ian, Itoh, Hiroshi, Licchelli, Domenico, Dvorak, Shawn, Sabo, Richard, Ögmen, Yenal, Starkey, Donn R., Nelson, Peter, de Miguel, Enrique, Galdies, Charles, Menzies, Kenneth, Kiyota, Seiichiro, Oksanen, Arto, Pickard, Roger D., Zubareva, Alexandra M., Wenzel, Klaus, Denisenko, Denis
Publikováno v:
Variable Star Bulletin, 74, 2021
How a black hole accretes matter and how this process is regulated are fundamental but unsolved questions in astrophysics. In transient black-hole binaries, a lot of mass stored in an accretion disk is suddenly drained to the central black hole becau
Externí odkaz:
http://arxiv.org/abs/2107.03681
Autor:
Kostov, Veselin B., Powell, Brian P., Orosz, Jerome A., Welsh, William F., Cochran, William, Collins, Karen A., Endl, Michael, Hellier, Coel, Latham, David W., MacQueen, Phillip, Pepper, Joshua, Quarles, Billy, Sairam, Lalitha, Torres, Guillermo, Wilson, Robert F., Bergeron, Serge, Boyce, Pat, Bieryla, Allyson, Buchheim, Robert, Christiansen, Caleb Ben, Ciardi, David R., Collins, Kevin I., Conti, Dennis M., Dixon, Scott, Guerra, Pere, Haghighipour, Nader, Herman, Jeffrey, Hintz, Eric G., Howard, Ward S., Jensen, Eric L. N., Kielkopf, John F., Kruse, Ethan, Law, Nicholas M., Martin, David, Maxted, Pierre F. L., Montet, Benjamin T., Murgas, Felipe, Nelson, Matt, Olmschenk, Greg, Otero, Sebastian, Quimby, Robert, Richmond, Michael, Schwarz, Richard P., Shporer, Avi, Stassun, Keivan G., Stephens, Denise C., Triaud, Amaury H. M. J., Ulowetz, Joe, Walter, Bradley S., Wiley, Edward, Wood, David, Yenawine, Mitchell, Agol, Eric, Barclay, Thomas, Beatty, Thomas G., Boisse, Isabelle, Caldwell, Douglas A., Christiansen, Jessie, Colon, Knicole D., Deleuil, Magali, Doyle, Laurance, Fabrycky, Daniel, Fausnaugh, Michael, Furesz, Gabor, Gilbert, Emily A., Hebrard, Guillaume, James, David J., Jenkins, Jon, Kane, Stephen R., Kidwell Jr., Richard C., Kopparapu, Ravi, Li, Gongjie, Lissauer, Jack J., Lund, Michael B., Majewski, Steve, Mazeh, Tsevi, Quinn, Samuel N., Quintana, Elisa, Ricker, George, Rodriguez, Joseph E., Rowe, Jason, Santerne, Alexander, Schlieder, Joshua, Seager, Sara, Standing, Matthew R., Stevens, Daniel J., Ting, Eric B., Vanderspek, Roland, Winn, Joshua N.
We report the first discovery of a transiting circumbinary planet detected from a single sector of TESS data. During Sector 21, the planet TIC 172900988b transited the primary star and then 5 days later it transited the secondary star. The binary is
Externí odkaz:
http://arxiv.org/abs/2105.08614
Autor:
Tampo, Yusuke, Naoto, Kojiguchi, Isogai, Keisuke, Kato, Taichi, Kimura, Mariko, Wakamatsu, Yasuyuki, Nogami, Daisaku, Vanmunster, Tonny, Tordai, Tamás, Akazawa, Hidehiko, Mugas, Felipe, Nishiumi, Taku, Béjar, Víctor J. S., Kawauchi, Kiyoe, Crouzet, Nicolas, Watanabe, Noriharu, Casasayas-Barris, Núria, Terada, Yuka, Fukui, Akihiko, Narita, Norio, Palle, Enric, Tamura, Motohide, Kusakabe, Nobuhiko, Alonso, Roi, Itoh, Hiroshi, Sokolovsky, Kirill, McIntyre, Brandon, Leahy-McGregor, Jesse, Brincat, Stephen M., Dubovsky, Pavol A., Medulka, Tomáš, Kudzej, Igor, Pavlenko, Elena P., Antonyuk, Kirill A., Pit, Nikolaj V., Antonyuk, Oksana I., Babina, Julia V., Baklanov, Aleksei V., Sklyanov, Aleksander S., Zubareva, Alexandra M., Belinski, Aleksandr A., Dodin, Alexandr V., Burlak, Marina A., Ikonnikova, Natalia P., Mishin, Egor O., Potanin, Sergey A., Miller, Ian, Richmond, Michael, Pickard, Roger D., Galdies, Charles, Mizutani, Masanori, Menzies, Kenneth, Stone, Geoffrey, Ruiz, Javier
We report photometric and spectroscopic observations and analysis of the 2019 superoutburst of TCP J21040470+4631129. This object showed a 9-mag superoutburst with early superhumps and ordinary superhumps, which are the features of WZ Sge-type dwarf
Externí odkaz:
http://arxiv.org/abs/2004.10508
The size and structure of the dusty circumnuclear torus in active galactic nuclei (AGN) can be investigated by analyzing the temporal response of the torus's infrared (IR) dust emission to variations in the AGN ultraviolet/optical luminosity. This me
Externí odkaz:
http://arxiv.org/abs/2002.12823
Publikováno v:
In Journal of Organometallic Chemistry 1 November 2023 1000