Scaling slowly rotating asteroids by stellar occultations

Autor: Marciniak, A., Ďurech, J., Choukroun, A., Hanuš, J., Ogłoza, W., Szakáts, R., Molnár, L., Pál, A., Monteiro, F., Frappa, E., Beisker, W., Pavlov, H., Moore, J., Adomavičienė, R., Aikawa, R., Andersson, S., Antonini, P., Argentin, Y., Asai, A., Assoignon, P., Barton, J., Baruffetti, P., Bath, K. L., Behrend, R., Benedyktowicz, L., Bernasconi, L., Biguet, G., Billiani, M., Błażewicz, D., Boninsegna, R., Borkowski, M., Bosch, J., Brazill, S., Bronikowska, M., Bruno, A., Bąk, M. Butkiewicz, Caron, J., Casalnuovo, G., Castellani, J. J., Ceravolo, P., Conjat, M., Delincak, P., Delpau, J., Demeautis, C., Demirkol, A., Dróżdż, M., Duffard, R., Durandet, C., Eisfeldt, D., Evangelista, M., Fauvaud, S., Fauvaud, M., Ferrais, M., Filipek, M., Fini, P., Fukui, K., Gährken, B., Geier, S., George, T., Goffin, B., Golonka, J., Goto, T., Grice, J., Guhl, K., Halíř, K., Hanna, W., Harman, M., Hashimoto, A., Hasubick, W., Higgins, D., Higuchi, M., Hirose, T., Hirsch, R., Hofschulz, O., Horaguchi, T., Horbowicz, J., Ida, M., Ignácz, B., Ishida, M., Isobe, K., Jehin, E., Joachimczyk, B., Jones, A., Juan, J., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kasebe, H., Kattentidt, B., Kim, D. -H., Kim, M. -J., Kitazaki, K., Klotz, A., Komraus, M., Konstanciak, I., Tóth, R. Könyves, Kouno, K., Kowald, E., Krajewski, J., Krannich, G., Kreutzer, A., Kryszczyńska, A., Kubánek, J., Kudak, V., Kugel, F., Kukita, R., Kulczak, P., Lazzaro, D., Licandro, J., Livet, F., Maley, P., Manago, N., Mánek, J., Manna, A., Matsushita, H., Meister, S., Mesquita, W., Messner, S., Michelet, J., Michimani, J., Mieczkowska, I., Morales, N., Motyliński, M., Murawiecka, M., Newman, J., Nikitin, V., Nishimura, M., Oey, J., Oszkiewicz, D., Owada, M., Pakštienė, E., Pawłowski, M., Pereira, W., Perig, V., Perła, J., Pilcher, F., Podlewska-Gaca, E., Polák, J., Polakis, T., Polińska, M., Popowicz, A., Richard, F., Rives, J. J., Rodrigues, T., Rogiński, Ł., Rondón, E., Rottenborn, M., Schäfer, R., Schnabel, C., Schreurs, O., Selva, A., Simon, M., Skiff, B., Skrutskie, M., Skrzypek, J., Sobkowiak, K., Sonbas, E., Sposetti, S., Stuart, P., Szyszka, K., Terakubo, K., Thomas, W., Trela, P., Uchiyama, S., Urbanik, M., Vaudescal, G., Venable, R., Watanabe, Ha., Watanabe, Hi., Winiarski, M., Wróblewski, R., Yamamura, H., Yamashita, M., Yoshihara, H., Zawilski, M., Zelený, P., Żejmo, M., Żukowski, K., Żywica, S.

Publikováno v: A&A 679, A60 (2023)

As evidenced by recent survey results, majority of asteroids are slow rotators (P>12 h), but lack spin and shape models due to selection bias. This bias is skewing our overall understanding of the spins, shapes, and sizes of asteroids, as well as of

Externí odkaz: http://arxiv.org/abs/2310.08995

A multi-epoch, multi-wavelength study of the classical FUor V1515 Cyg approaching quiescence

Autor: Szabó, Zs. M., Kóspál, Á., Ábrahám, P., Park, S., Siwak, M., Green, J. D., Pál, A., Acosta-Pulido, J. A., Lee, J. -E., Ibrahimov, M., Grankin, K., Kovács, B., Bora, Zs., Bódi, A., Cseh, B., Csörnyei, G., Drózdz, Marek, Hanyecz, O., Ignácz, B., Kalup, Cs., Könyves-Tóth, R., Krezinger, M., Kriskovics, L., Ogloza, Waldemar, Ordasi, A., Sárneczky, K., Seli, B., Szakáts, R., Szing, A., Vida, K., Vinkó, J.

Historically, FU Orionis-type stars are low-mass, pre-main sequence stars. The members of this class experience powerful accretion outbursts and remain in an enhanced accretion state for decades or centuries. V1515 Cyg, a classical FUor, started brig

Externí odkaz: http://arxiv.org/abs/2206.12446

V899 Mon: a peculiar eruptive young star close to the end of its outburst

Autor: Park, Sunkyung, Kóspál, Ágnes, de Miera, Fernando Cruz-Sáenz, Siwak, Michał, Dróżdż, Marek, Ignácz, Bernadett, Jaffe, Daniel T., Könyves-Tóth, Réka, Kriskovics, Levente, Lee, Jae-Joon, Lee, Jeong-Eun, Mace, Gregory N., Ogłoza, Waldemar, Pál, András, Potter, Stephen B., Szabó, Zsófia Marianna, Sefako, Ramotholo, Worters, Hannah L.

V899 Mon is an eruptive young star showing characteristics of both FUors and EXors. It reached a peak brightness in 2010, then briefly faded in 2011, followed by a second outburst. We conducted multi-filter optical photometric monitoring, as well as

Externí odkaz: http://arxiv.org/abs/2109.11283

The Peculiar Transient AT2018cow: A Possible Origin of A Type Ibn/IIn Supernova

Autor: Xiang, Danfeng, Wang, Xiaofeng, Lin, Weili, Mo, Jun, Lin, Han, Burke, Jamison, Hiramatsu, Daichi, Hosseinzadeh, Griffin, Howell, D. Andrew, McCully, Curtis, Valenti, Stefan, Vinkó, József, Wheeler, J. Craig, Ehgamberdiev, Shuhrat A., Mirzaqulov, Davron, Bódi, Attila, Bognár, Zsófia, Cseh, Borbála, Hanyecz, Ottó, Ignácz, Bernadett, Kalup, Csilla, Könyves-Tóth, Réka, Kriskovics, Levente, Ordasi, András, Pál, András, Sárneczky, Krisztián, Seli, Bálint, Szakáts, Róbert, Arranz-Heras, T., Benavides-Palencia, R., Cejudo-Martínez, D., De la Fuente-Fernández, P., Escartín-Pérez, A., la Cuesta, F. García-De, González-Carballo, J. L., González-Farfán, R., Limón-Martínez, F., Mantero, A., Naves-Nogués, R., Morales-Aimar, M., Ruíz-Ruíz, V. R., Soldán-Alfaro, F. C., Valero-Pérez, J., Violat-Bordonau, F., Zhang, Tianmeng, Zhang, Jujia, Li, Xue, Chen, Zhihao, Sai, Hanna, Li, Wenxiong

We present our photometric and spectroscopic observations on the peculiar transient AT2018cow. The multi-band photometry covers from peak to $\sim$70 days and the spectroscopy ranges from 5 to $\sim$50 days. The rapid rise ($t_{\mathrm{r}}$$\lesssim$

Externí odkaz: http://arxiv.org/abs/2101.08009

Subarachnoid Hemorrhage Depletes Calcitonin Gene-Related Peptide Levels of Trigeminal Neurons in Rat Dura Mater

Autor: Thannoon Masood, Szandra Lakatos, Gyöngyi Kis, Melissza Ignácz, Ferenc Domoki, Judit Rosta

Publikováno v: Cells, Vol 13, Iss 8, p 653 (2024)

Subarachnoid hemorrhage (SAH) remains a major cause of cerebrovascular morbidity, eliciting severe headaches and vasospasms that have been shown to inversely correlate with vasodilator calcitonin gene-related peptide (CGRP) levels. Although dura mate

Externí odkaz: https://doaj.org/article/3e3b367f52c646faa53db6e6a1e93465