Results 111 to 120 of about 31,180 (215)
Discovery and Extensive Follow-up of SN 2024ggi, a Nearby Type IIP Supernova in NGC 3621
The Astrophysical JournalWe present the discovery and early observations of the nearby Type II supernova (SN) 2024ggi in NGC 3621 at 6.64 ± 0.3 Mpc. The SN was caught $5.{8}_{-2.9}^{+1.9}$ hr after its explosion by the ATLAS survey.Ting-Wan Chen, Sheng Yang, Shubham Srivastav, Takashi J. Moriya, Stephen J. Smartt, Sofia Rest, Armin Rest, Hsing Wen Lin, Hao-Yu Miao, Yu-Chi Cheng, Amar Aryan, Chia-Yu Cheng, Morgan Fraser, Li-Ching Huang, Meng-Han Lee, Cheng-Han Lai, Yu-Hsuan Liu, Aiswarya Sankar.K, Ken W. Smith, Heloise F. Stevance, Ze-Ning Wang, Joseph P. Anderson, Charlotte R. Angus, Thomas de Boer, Kenneth Chambers, Hao-Yuan Duan, Nicolas Erasmus, Michael Fulton, Hua Gao, Joanna Herman, Wei-Jie Hou, Hsiang-Yao Hsiao, Mark E. Huber, Chien-Cheng Lin, Hung-Chin Lin, Eugene A. Magnier, Ka Kit Man, Thomas Moore, Chow-Choong Ngeow, Matt Nicholl, Po-Sheng Ou, Giuliano Pignata, Yu-Chien Shiau, Julian Silvester Sommer, John L. Tonry, Xiao-Feng Wang, Richard Wainscoat, David R. Young, You-Ting Yeh, Jujia Zhang +49 moredoaj +1 more sourceStrangeness in Compact Stars
, 2010 We discuss the impact of strange hadrons, in particular hyperons, on the
gross features of compact stars and on core-collapse supernovae. Hyperons are
likely to be the first exotic species which appears around twice normal nuclear
matter density in the ...Aichelin, Ambartsumyan, Andersson, Balberg, Baldo, Baldo, Champion, Chatterjee, Dexheimer, Drago, Ellis, Freire, Fuchs, Förster, Glendenning, Glendenning, Gusakov, Haensel, Hanauske, Hartnack, Hofmann, Huber, Ishizuka, Janka, Jones, Jones, Jürgen Schaffner-Bielich, Kalogera, Knorren, Lattimer, Lindblom, Mintz, Nayyar, Nice, Nishizaki, Oppenheimer, Page, Pal, Rhoades, Sagert, Sagert, Sagert, Sagert, Schaab, Schaffner, Schaffner-Bielich, Schramm, Schulze, Sturm, Sumiyoshi, Takatsuka, van Dalen, Vidana, Vidaña, Weber, Weisberg, Zhou, Đapo +57 morecore +1 more sourceCharacterizing the Rapid Hydrogen Disappearance in SN 2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties
The Astrophysical JournalWe present optical and near-infrared (NIR) observations of SN 2022crv, a stripped-envelope supernova in NGC 3054, discovered within 12 hr of explosion by the Distance Less Than 40 Mpc Survey.Yize Dong, Stefano Valenti, Chris Ashall, Marc Williamson, David J. Sand, Schuyler D. Van Dyk, Alexei V. Filippenko, Saurabh W. Jha, Michael Lundquist, Maryam Modjaz, Jennifer E. Andrews, Jacob E. Jencson, Griffin Hosseinzadeh, Jeniveve Pearson, Lindsey A. Kwok, Teresa Boland, Eric Y. Hsiao, Nathan Smith, Nancy Elias-Rosa, Shubham Srivastav, Stephen Smartt, Michael Fulton, WeiKang Zheng, Thomas G. Brink, Melissa Shahbandeh, K. Azalee Bostroem, Emily Hoang, Daryl Janzen, Darshana Mehta, Nicolas Meza, Manisha Shrestha, Samuel Wyatt, Katie Auchettl, Christopher R. Burns, Joseph Farah, Lluís Galbany, Estefania Padilla Gonzalez, Joshua Haislip, Jason T. Hinkle, D. Andrew Howell, Thomas De Jaeger, Vladimir Kouprianov, Sahana Kumar, Jing Lu, Curtis McCully, Shane Moran, Nidia Morrell, Megan Newsome, Craig Pellegrino, Abigail Polin, Daniel E. Reichart, B. J. Shappee, Maximilian D. Stritzinger, Giacomo Terreran, M. A. Tucker +54 moredoaj +1 more sourceThe Cosmic Stellar Birth and Death Rates
, 2006 The cosmic stellar birth rate can be measured by standard astronomical
techniques. It can also be probed via the cosmic stellar death rate, though
until recently, this was much less precise.Ahn, Ando, Ando, Beacom, Bionta, Bisnovatyi-Kogan, Clayton, Fukugita, Hirata, Hopkins, John F. Beacom, Krauss, Malek, Milne, Mirizzi, Schiminovich, Strigari, Strigari, Watanabe, Woosley, Yoshida, Zhang, Zhang +22 morecore +2 more sourcesOptical and Near-infrared Nebular-phase Spectroscopy of SN 2024ggi: Constraints on the Structure of the Inner Ejecta, Progenitor Mass, and Dust
The Astrophysical JournalWe present optical and near-infrared (NIR) spectroscopic observations of the nearby Type II supernova SN 2024ggi ranging from 250 to 581 days after the explosion.Emilio Hueichapán, Régis Cartier, Jose L. Prieto, Carlos Contreras, Aleksandar Cikota, Thallis Pessi, Franz E. Bauer, Giuliano Pignata, Camila Cardenas, Sethulakshmi Vazhayil +9 moredoaj +1 more sourceHubble Space Telescope Deep Upper Limits Rule out a Surviving Massive Binary Companion to the Type Ic Supernova 2012fh
The Astrophysical JournalCurrent explanations of the mass-loss mechanism for stripped-envelope supernovae (SNe) remain divided between single and binary progenitor systems. Here we obtain deep ultraviolet (UV) imaging with the Hubble Space Telescope (HST) of the Type Ic SN ...Benjamin F. Williams, Emmanouil Zapartas, Ori D. Fox, K. Azalee Bostroem, Jianing Su, Brad Koplitz, Schuyler D. Van Dyk, Maria R. Drout, Dimitris Souropanis, Dan Milisavljevic, Stuart D. Ryder, Selma E. de Mink, Nathan Smith, Andrew Dolphin, Alexei V. Filippenko, Jeff J. Andrews, Max M. Briel, Seth Gossage, Matthias U. Kruckow, Camille Liotine, Philipp M. Srivastava, Elizabeth Teng +21 moredoaj +1 more sourceExplosive nucleosynthesis in core-collapse supernovae
, 2010 The specific mechanism and astrophysical site for the production of half of
the elements heavier than iron via rapid neutron capture (r-process) remains to
be found.Almudena Arcones, Aoki W, Arcones A, Arcones A, Arcones A, Farouqi K, Freiburghaus C, Fröhlich C, Goriely S, Hoffman R D, Ishimaru Y, Ishimaru Y, Montes F, NuDat2, Otsuki K, Otsuki K, Pruet J, Qian Y Z, Qian Y Z, Qian Y Z, Thompson T A, Travaglio C, Wanajo S, Wanajo S, Wanajo S, Wanajo S, Wasserburg G J, Wasserburg G J, Witti J +28 morecore +1 more source
