Zobrazeno 1 - 10
of 28 799
pro vyhledávání: '"Vela, P."'
Autor:
Rajohnson, Sambatriniaina H. A., Kraan-Korteweg, Renée C., Frank, Bradley S., Chen, Hao, Staveley-Smith, Lister, Serra, Paolo, Steyn, Nadia, Kurapati, Sushma, Pisano, D. J., Goedhart, Sharmila
We conducted the MeerKAT Vela Supercluster survey, named Vela$-$HI, to bridge the gap between the Vela SARAO MeerKAT Galactic Plane Survey (Vela$-$SMGPS, $-2^{\circ} \leq b \leq 1^{\circ}$), and optical and near-infrared spectroscopic observations of
Externí odkaz:
http://arxiv.org/abs/2411.07084
The Vela pulsar (J0835-4510) is known to exhibit variations in Faraday rotation and dispersion on multi-decade timescales due to the changing sightline through the surrounding Vela supernova remnant and the Gum Nebula. Until now, variations in Farada
Externí odkaz:
http://arxiv.org/abs/2411.00602
Autor:
Deng, Wei, Xie, Fei, Liu, Kuan, Ge, Mingyu, Tuo, Youli, La Monaca, Fabio, Di Marco, Alessandro, Liang, En-wei
Polarization measurements provide insight into the magnetic field, a critical aspect of the dynamics and emission properties around the compact object. In this paper, we present the polarized magnetic field of the Crab outer torus and the Vela arc ut
Externí odkaz:
http://arxiv.org/abs/2410.05622
Autor:
Abalo, L., Kretschmar, P., Fürst, F., Diez, C. M., Mellah, I. El, Grinberg, V., Guainazzi, M., Martínez-Núñez, S., Manousakis, A., Amato, R., Zhou, M., Beijersbergen, M. W.
Publikováno v:
A&A 692, A188 (2024)
Strong stellar winds are an important feature in wind-accreting high-mass X-ray binary (HMXB) systems, providing insights into stellar evolution and their impact on surrounding environments. However, the long-term evolution and temporal variability o
Externí odkaz:
http://arxiv.org/abs/2410.21456
Autor:
Prokhorov, Dmitry A., Yang, Yi-Jung, Ferrazzoli, Riccardo, Vink, Jacco, Slane, Patrick, Costa, Enrico, Silvestri, Stefano, Zhou, Ping, Bucciantini, Niccolò, Di Marco, Alessandro, Weisskopf, Martin C., Baldini, Luca, Doroshenko, Victor, Ehlert, Steven R., Heyl, Jeremy, Kaaret, Philip, Kim, Dawoon E., Marin, Frédéric, Mizuno, Tsunefumi, Ng, Chi-Yung, Pesce-Rollins, Melissa, Sgrò, Carmelo, Soffitta, Paolo, Swartz, Douglas A., Tamagawa, Toru, Xie, Fei, Agudo, Iván, Antonelli, Lucio A., Bachetti, Matteo, Baumgartner, Wayne H., Bellazzini, Ronaldo, Bianchi, Stefano, Bongiorno, Stephen D., Bonino, Raffaella, Brez, Alessandro, Capitanio, Fiamma, Castellano, Simone, Cavazzuti, Elisabetta, Chen, Chien-Ting, Ciprini, Stefano, De Rosa, Alessandra, Del Monte, Ettore, Di Gesu, Laura, Di Lalla, Niccolò, Donnarumma, Immacolata, Dovčiak, Michal, Enoto, Teruaki, Evangelista, Yuri, Fabiani, Sergio, García, Javier A., Gunji, Shuichi, Iwakiri, Wataru, Jorstad, Svetlana G., Karas, Vladimir, Kislat, Fabian, Kitaguchi, Takao, Kolodziejczak, Jeffery J., Krawczynski, Henric, La Monaca, Fabio, Latronico, Luca, Liodakis, Ioannis, Maldera, Simone, Manfreda, Alberto, Marinucci, Andrea, Marscher, Alan P., Marshall, Herman L., Massaro, Francesco, Matt, Giorgio, Mitsuishi, Ikuyuki, Muleri, Fabio, Negro, Michela, O'Dell, Stephen L., Omodei, Nicola, Oppedisano, Chiara, Papitto, Alessandro, Pavlov, George G., Peirson, Abel L., Perri, Matteo, Petrucci, Pierre-Olivier, Pilia, Maura, Possenti, Andrea, Poutanen, Juri, Puccetti, Simonetta, Ramsey, Brian D., Rankin, John, Ratheesh, Ajay, Roberts, Oliver J., Romani, Roger W., Spandre, Gloria, Tavecchio, Fabrizio, Taverna, Roberto, Tawara, Yuzuru, Tennant, Allyn F., Thomas, Nicholas E., Tombesi, Francesco, Trois, Alessio, Tsygankov, Sergey S., Turolla, Roberto, Wu, Kinwah, Zane, Silvia
Synchrotron X-ray emission has been detected from nearly a dozen young supernova remnants (SNRs). X-rays of synchrotron origin exhibit linear polarization in a regular, non-randomly oriented magnetic field. The significant polarized X-ray emission fr
Externí odkaz:
http://arxiv.org/abs/2410.20582
Autor:
Yang, Dongting, Liu, HongLi, Liu, Tie, Tej, Anandmayee, Liu, Xunchuan, He, Jinhua, Garay, Guido, Stutz, Amelia, Zhu, Lei, Qin, Sheng-Li, Xu, Fengwei, Li, Pak-Shing, Juvela, Mika, Garcia, Pablo, Goldsmith, Paul F., Zhang, Siju, Tang, Xindi, Sanhueza, Patricio, Li, Shanghuo, Lee, Chang Won, Das, Swagat Ranjan, Jiao, Wenyu, Mai, Xiaofeng, Gorai, Prasanta, Zhang, Yichen, Ren, Zhiyuan, Toth, L. Viktor, Hwang, Jihye, Bronfman, Leonardo, Tatematsu, Kenichi, Dewangan, Lokesh, Chibueze, James O., Zhang, Suinan, Wu, Gang, Xie, Jinjin
In this paper, we present a detailed analysis of the IRS 17 filament within the intermediate-mass protocluster IRAS 08448-4343 (of $\sim\,10^3\,\rm L_{\odot}$), using ALMA data from the ATOMS 3-mm and QUARKS 1.3-mm surveys. The IRS 17 filament, which
Externí odkaz:
http://arxiv.org/abs/2410.15333
Autor:
Soker, Noam, Shishkin, Dmitry
We identify an S-shaped main-jet axis in the Vela core-collapse supernova (CCSN) remnant (CCSNR) that we attribute to a pair of precessing jets, one of the tens of pairs of jets that exploded the progenitor of Vela according to the jittering jets exp
Externí odkaz:
http://arxiv.org/abs/2409.02626
Autor:
Ming, Jing, Papa, Maria Alessandra, Eggenstein, Heinz-Bernd, Beheshtipour, Banafsheh, Machenschalk, Bernd, Prix, Reinhard, Allen, Bruce, Bensch, Maximillian
We perform a search for continuous nearly monochromatic gravitational waves from the central compact objects associated with the supernova remnants Vela Jr. and G347.3 using LIGO O2 and O3 public data. Over $10^{18}$ different waveforms are considere
Externí odkaz:
http://arxiv.org/abs/2408.14573
Autor:
Dinkel, Holly M., Cornelius, Jason K.
The UN Office of Outer Space Affairs identifies synergy of space development activities and international cooperation through data and infrastructure sharing in their Sustainable Development Goal 17 (SDG17). Current multilateral space exploration par
Externí odkaz:
http://arxiv.org/abs/2408.04730
To learn more about the properties of the Vela Supercluster (VSCL) located behind the Milky Way at $cz\sim 18000$~km~s$^{-1}$, we determined the $K_s$-band Luminosity Function (LF) of VC04, the richest known galaxy cluster in the VSCL, and two other
Externí odkaz:
http://arxiv.org/abs/2407.14425