The Origin and Evolution of the Normal Type Ia SN 2018aoz with Infant-phase Reddening and Excess Emission by Yuan Qi Ni, Dae-Sik Moon, Maria R. Drout, Abigail Polin, David J. Sand, Santiago González-Gaitán, Sang Chul Kim, Youngdae Lee, Hong Soo Park, D. Andrew Howell, Peter E. Nugent, Anthony L. Piro, Peter J. Brown, Lluís Galbany, Jamison Burke, Daichi Hiramatsu, Griffin Hosseinzadeh, Stefano Valenti, Niloufar Afsariardchi, Jennifer E. Andrews, John Antoniadis, Rachael L. Beaton, K. Azalee Bostroem, Raymond G. Carlberg, S. Bradley Cenko, Sang-Mok Cha, Yize Dong, Avishay Gal-Yam, Joshua Haislip, Thomas W.-S. Holoien, Sean D. Johnson, Vladimir Kouprianov, Yongseok Lee, Christopher D. Matzner, Nidia Morrell, Curtis McCully, Giuliano Pignata, Daniel E. Reichart, Jeffrey Rich, Stuart D. Ryder, Nathan Smith, Samuel Wyatt, Sheng Yang

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The Progenitors of Superluminous Type Ia Supernovae by Margot Fitz Axen, Peter Nugent

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The Early Light Curve of the Type Ia Supernova 2021hpr in NGC 3147: Progenitor Constraints with the Companion Interaction Model by Gu Lim, Myungshin Im, Gregory S. H. Paek, Sung-Chul Yoon, Changsu Choi, Sophia Kim, J. Craig Wheeler, Benjamin P. Thomas, Jozsef Vinkó, Dohyeong Kim, Jinguk Seo, Wonseok Kang, Taewoo Kim, Hyun-Il Sung, Yonggi Kim, Joh-Na Yoon, Haeun Kim, Jeongmook Kim, Hana Bae, Shuhrat Ehgamberdiev, Otabek Burhonov, Davron Mirzaqulov

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The Binary and the Disk: The Beauty is Found within NGC3132 with JWST by Raghvendra Sahai, Valentin Bujarrabal, Guillermo Quintana-Lacaci, Nicole Reindl, Griet Van de Steene, Carmen Sánchez Contreras, Michael E. Ressler

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Single Millisecond Pulsars from Dynamical Interaction Processes in Dense Star Clusters by Claire S. Ye, Kyle Kremer, Scott M. Ransom, Frederic A. Rasio

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Prospects for Detecting Fast Radio Bursts in the Globular Clusters of Nearby Galaxies by Kyle Kremer, Dongzi Li, Wenbin Lu, Anthony L. Piro, Bing Zhang

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WOCS 4540: Detailed Analysis of a very Long Orbital Period Blue Straggler by Meng Sun, Robert D. Mathieu

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Precise Age for the Binary Star System 12 Com in the Coma Berenices Cluster by Rex Lam, Eric L. Sandquist, Gail H. Schaefer, Christopher D. Farrington, John D. Monnier, Narsireddy Anugu, Cyprien Lanthermann, Robert Klement, Jacob Ennis, Benjamin R. Setterholm, Tyler Gardner, Stefan Kraus, Claire L. Davies, Jerome A. Orosz

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Nucleus-Acoustic Solitary Waves in Warm Degenerate Magneto-Rotating Quantum Plasmas by Jhorna Akter, A A Mamun

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Compact objects in close orbits as gravitational wave sources: Formation scenarios and properties by Zhenwei Li, Xuefei Chen

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Does Nature Allow the Formation of Ultra-compact Black Hole X-Ray Binaries via the Accretion-induced Collapse of Neutron Stars? by Hai-Liang Chen, Thomas M. Tauris, Xuefei Chen, Zhanwen Han

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Giant Planet Engulfment by Evolved Giant Stars: Light Curves, Asteroseismology, and Survivability by Christopher E. O’Connor, Lars Bildsten, Matteo Cantiello, Dong Lai

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Stark Broadening of Co II Lines in Stellar Atmospheres by Zlatko Majlinger, Milan S. Dimitrijević, Vladimir A. Srećković

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SCATTER: A New Common Envelope Formalism by Rosanne Di Stefano, Matthias U. Kruckow, Yan Gao, Patrick G. Neunteufel, Chiaki Kobayashi

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8.962 General Relativity, Spring 2002 by Bertschinger, Edmund W.

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8.282J / 12.402J Introduction to Astronomy, Spring 2003 by Rappaport, S. A., 1942-, Elliot, James, 1943-

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Recurrent novae: Type Ia supernovae in the making by Hachisu, I, Kato, M

“…The mass of the white dwarf ranges from 1.35-1.37 M. for seven recurrent novae except for T Pyx which has a less massive white dwarf of 1.2 M.. …”

Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe. by Li, W, Bloom, J, Podsiadlowski, P, Miller, A, Cenko, S, Jha, S, Sullivan, M, Howell, D, Nugent, P, Butler, N, Ofek, E, Kasliwal, M, Richards, J, Stockton, A, Shih, H, Bildsten, L, Shara, M, Bibby, J, Filippenko, A, Ganeshalingam, M, Silverman, J, Kulkarni, SR, Law, N, Poznanski, D, Quimby, R

“…There are two classes of models: double-degenerate (involving two white dwarfs in a close binary system) and single-degenerate models. …”

Laboratory analogue of a supersonic accretion column in a binary star system. by Cross, J, Gregori, G, Foster, J, Graham, P, Bonnet-Bidaud, J, Busschaert, C, Charpentier, N, Danson, C, Doyle, H, Drake, R, Fyrth, J, Gumbrell, E, Koenig, M, Krauland, C, Kuranz, C, Loupias, B, Michaut, C, Mouchet, M, Patankar, S, Skidmore, J, Spindloe, C, Tubman, E, Woolsey, N, Yurchak, R, Falize, É

“…For magnetic cataclysmic variable stars, material from a late, main sequence star is pulled onto a highly magnetized (B>10 MG) white dwarf. The magnetic field is sufficiently large to direct the flow as an accretion column onto the poles of the white dwarf, a star subclass known as AM Herculis. …”

Laboratory analogue of a supersonic accretion column in a binary star system. by Cross, J, Gregori, G, Foster, J, Graham, P, Bonnet-Bidaud, J, Busschaert, C, Charpentier, N, Danson, C, Doyle, H, Drake, R, Fyrth, J, Gumbrell, E, Koenig, M, Krauland, C, Kuranz, C, Loupias, B, Michaut, C, Mouchet, M, Patankar, S, Skidmore, J, Spindloe, C, Tubman, E, Woolsey, N, Yurchak, R, Falize, É

“…For magnetic cataclysmic variable stars, material from a late, main sequence star is pulled onto a highly magnetized (B>10 MG) white dwarf. The magnetic field is sufficiently large to direct the flow as an accretion column onto the poles of the white dwarf, a star subclass known as AM Herculis. …”