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相关论文: The red supergiant progenitor luminosity problem

200 篇论文

Red supergiants (RSGs), which are progenitors of hydrogen-rich Type II supernovae (SNe), have been known to pulsate from both observations and theory. The pulsations can be present at core collapse and affect the resulting SN. However, SN…

太阳与恒星天体物理 · 物理学 2025-11-12 V. A. Bronner , E. Laplace , F. R. N. Schneider , Ph. Podsiadlowski

UVOIR bolometric light curves provide valuable insight into the nature of type Ia supernovae. We present an analysis of sixteen well-observed SNe Ia. Constraints are placed on several global parameters concerning the progenitor system,…

天体物理学 · 物理学 2009-11-11 Maximilian Stritzinger , Bruno Leibundgut , Stefanie Walch , Gertrud Contardo

We explore properties of Type Ib and IIb SN progenitors that are produced by stable mass transfer in binary systems, using a new grid of stellar evolution models from an initial primary mass in the range of 10 - 18 $\mathrm{M_\odot}$ at…

太阳与恒星天体物理 · 物理学 2017-05-03 Sung-Chul Yoon , Luc Dessart , Alejandro Clocchiatti

Masses and progenitor evolutionary states of TypeII supernovae remain almost unconstrained by direct observations. Only one robust observation of a progenitor (SN1987A) and one plausible observation (SN1993J) are available. Neither matched…

天体物理学 · 物理学 2016-08-30 S. J. Smartt , G. F. Gilmore , N. Trentham , C. A. Tout , C. M. Frayn

The progenitors of Type IIP supernovae (SNe) are known to be red supergiants, but their properties are not well determined. We employ hydrodynamical modelling to investigate the explosion characteristics of eight Type IIP supernovae, and…

高能天体物理现象 · 物理学 2019-06-19 Wilson Ricks , Vikram V. Dwarkadas

For typical models of binary statistics, 50-70% of core-collapse supernova (ccSN) progenitors are members of a stellar binary at the time of the explosion. Independent of any consequences of mass transfer, this has observational…

太阳与恒星天体物理 · 物理学 2014-11-20 C. S. Kochanek

Thirteen explosion sites of type II-P and II-L supernovae in nearby galaxies have been observed using integral field spectroscopy, enabling both spatial and spectral study of the explosion sites. We used the properties of the parent stellar…

We present adaptive optics imaging of the core collapse supernova (SN) 2009md, which we use together with archival \emph{Hubble Space Telescope} data to identify a coincident progenitor candidate. We find the progenitor to have an absolute…

Observations of type II supernova early light, from breakout until recombination, can be used to constrain the explosion energy and progenitor properties. Currently available for this purpose are purely analytic models, which are accurate…

高能天体物理现象 · 物理学 2016-10-19 Tomer Shussman , Roni Waldman , Ehud Nakar

We report our attempts to locate the progenitor of the type Ic SN 2004gt in NGC 4038. We use high resolution HST ACS images of SN 2004gt and have compared them with deep pre-explosion HST WFPC2 F336W, F439W, F555W and F814W images. We…

天体物理学 · 物理学 2009-11-13 Justyn R. Maund , Stephen Smartt , Francois Schweizer

We present a systematic study of Type II supernovae (SNe II) originating from progenitors with effective temperatures ($T_{\rm eff}$) and luminosities closely resembling red supergiants (RSGs) observed in pre-SN images and in the Galaxy.…

高能天体物理现象 · 物理学 2024-09-16 Qiliang Fang , Keiichi Maeda , Haonan Ye , Takashi Moriya , Tatsuya Matsumoto

The progenitors of hydrogen-poor core-collapse supernovae (SNe) of types Ib, Ic and IIb are believed to have shed their outer hydrogen envelopes either by extremely strong stellar winds, characteristic of classical Wolf-Rayet stars, or by…

高能天体物理现象 · 物理学 2016-02-03 T. Heikkilä , S. Tsygankov , S. Mattila , J. J. Eldridge , M. Fraser , J. Poutanen

We compile a catalog of 578 highly probable and 62 likely red supergiants (RSGs) of the Milky Way, which represents the largest list of Galactic RSG candidates designed for continuous follow-up to date. We match distances measured by Gaia…

太阳与恒星天体物理 · 物理学 2024-05-08 Sarah Healy , Shunsaku Horiuchi , Marta Colomer Molla , Dan Milisavljevic , Jeff Tseng , Faith Bergin , Kathryn Weil , Masaomi Tanaka

In this study, we conduct a pilot program aimed at the red supergiant population of the Magellanic Clouds. We intend to extend the current known sample to the unexplored low end of the brightness distribution of these stars, building a more…

太阳与恒星天体物理 · 物理学 2015-05-27 Carlos González-Fernández , Ricardo Dorda , Ignacio Negueruela , Amparo Marco

We present a monitoring study of SN 2004A and probable discovery of a progenitor star in pre-explosion HST images. The photometric and spectroscopic monitoring of SN 2004A show that it was a normal Type II-P which was discovered in NGC 6207…

Type IIP Supernovae (SNe) are expected to arise from Red Supergiant stars (RSGs). These stars have observed mass-loss rates that span more than two orders of magnitude, from $< 10^{-6}$ solar masses yr$^{-1}$ to almost $ 10^{-4} $ solar…

高能天体物理现象 · 物理学 2015-06-18 Vikram V. Dwarkadas

We report on the direct detection and characterization of the probable red supergiant progenitor of the intermediate-luminosity Type II-Plateau (II-P) supernova (SN) 2012aw in the nearby (10.0 Mpc) spiral galaxy Messier 95 (M95; NGC 3351).…

The fate of massive stars with initial masses >8M$_\odot$ depends largely on the mass-loss rate (\mdot ) in the end stages of their lives. Red supergiants (RSGs) are the direct progenitors to Type II-P core collapse supernovae (SN), but…

太阳与恒星天体物理 · 物理学 2017-12-07 Emma R. Beasor , Ben Davies

We present photometric and spectroscopic data of the type II-P supernova 2003gd, which was discovered in M74 close to the end of its plateau phase. SN 2003gd is the first type II supernova to have a directly confirmed red supergiant…