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- 要約等...sses of binary stars. During a comm......ope phase, the stars temporarily sh...... cores of both stars orbiting inside the same comm...
- 内容細目... Phase I : the loss of orbital sta......ed 3.5. Energy losses : radiation ......olution due to mass loss 5.5. Increased mass loss before the RLO......verflow and L1 mass transfer 5.7. Mass loss via outer Lagr.......3. Transition from the plunge to ......ave we learned from one-dimensiona...... Mechanisms of mass ejection 8.1. ......tions 9.1. The mass of the initial......ed post-merger stars and their nebu.......5. Transients from CEE and stella...... mergers 10.6. Stars undergoing a common-envelope ...
- 件名Double stars--Evolution Ét......ion Galaxies & stars. SCIENCE--Physics--Astrophysi...
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- 件名Stars -- Congresses. Stars -- Evolution -- Congresses. Stars -- Clusters -- Congresses.
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- 要約等...predictions of mass-loss rates are important for massive-star evolut......redictions for mass-loss rates and wind......ates of O-type stars, while careful......of a grid of O-stars. The self-cons...... main-sequence stars, giants, and s...... dependence of mass-loss on both lumino......Similarly, the mass loss-luminosity rel...... relations for mass-loss rates and wind momenta of massive O-stars stars as functions o......simulations of massive stars.</jats:p>
- 参照Escape of cosmic rays from perpendicular shocks in the c...
- 並列タイトル等（連結）II. A grid of O-type stars in the Galaxy and the Magella...
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- 参照The Nearby Evolved Stars Survey II: Con...... first results from the James Cler...... CHANDRASEKHAR MASS LIMIT CO line ......tions of OH/IR stars in the inner G......acteristics of stars at the tip of the AGB Using b...
- 並列タイトル等（連結）II. CO line survey of evolved stars: derivation of mass-loss rate formulae
- 並列タイトル等II. CO line survey of evolved stars: derivation of mass-loss rate formulae
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- 要約等...ns of the high-mass X-ray binary C......star (41 solar masses) and the bla......hole (21 solar masses) are more massive than previo......t reduction in mass loss through winds ......s for stripped stars.</jats:p>
- 参照Observation of Gravitational Waves from Two Neutron Star–Black Hole C...
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- 要約等...t branch (AGB) stars often reveal n......utions (SEDs), mass estimates, and subsequent mass-loss rate (MLR) est......ulate emission from dusty envelope......lving the most massive envelopes a......apes originate from large differen......ptical depths. Massive spirals and......scs (with dust masses of 10<jats:s......ler than those from face-on struct......es of the same mass, while optical......0.5 times less massive than sphere.......05 times less massive than corres......e when derived from SED fitting.</jats:p>
- 参照CO line observations of OH/IR stars in the inner G......acteristics of stars at the tip of the AGB
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- 要約等...lic> > 6) supermassive black holes......e formation of massive seed BHs in......e formation of massive stars <jats:inline-f......leaving behind massive BHs without significant mass loss. We study the ......instability of massive stars with the zero-......equence (ZAMS) mass <jats:inline-f......lsation-driven mass loss prevents massive BH formatio......As the stellar mass and metallicit...... increase, the mass-loss rate increases......mula>. The RSG mass-loss rate is almost......mnant BHs more massive than <jats:...... conclude that massive merger products can seed m...
- 参照...ve Backgrounds from Coalescing Black Hole Binarie...
- 参照...upergiant protostars: do they grow supermassive by accretion? THE MASS SPECTRUM OF THE FIRST STARS The critical r......embryonic supermassive star in the......eeding of supermassive black holes......h of the First Stars in the Univers...... rotating supermassive stars including nucl......ation III very massive main-sequence stars due to the -mechanism Supermassive star format...... HUNDRED FIRST STARS</i>: PROTOSTEL...... AND THE FINAL MASSES Subaru High-......n of the first massive black holes Supermassive black hole ......s FORMATION OF MASSIVE PRIMORDIAL STARS: INTERMITTENT ...... WITH EPISODIC MASS ACCRETION Subaru High-z Explo...
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- 参照... Embedded in a Massive Circumstell......rst and second mass eruptions from progenitors of......ns of eruptive mass loss from progenitors of Type Ibn/IIn s...
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- 要約等... show that low-mass stars lose angular m......nds of sunlike stars with a range o......gular-momentum loss rate (torque) ......mula>. (2) The mass-loss rate saturates at <jats:inlin...
- 参照...n and Sun-like stars Reconstructing......ctive Sun-like Stars Using Solar Sc...... of solar-type stars Role of Longitudinal Waves in...
- 参照Do Kepler Superflare Stars Really Include......ating Sun-like Stars?—Results Using......ield Strengths from Zeeman–Doppler......for solar-like stars AGE DEPENDENCE......FOR SOLAR-TYPE STARS: A 3D STUDY Sl......es Theoretical mass loss rates of cool main-sequence stars Low-frequency ......tic Carpet New Mass-Loss Measurements from Astrospheric L......-SEQUENCE COOL STARS. I. INTRODUCTI......MPLICATIONS OF MASS AND ENERGY LOSS DUE TO CORONAL MASS EJECTIONS ON M......TICALLY ACTIVE STARS Asteroseismic ......f StellarWinds from Young Suns Ste......coronae of low-mass Population II/III stars The Small-scal......n in old field stars Circumstellar environment of ...
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- 要約等...cate that some massive stars may dynamicall......lose their own mass within decades...... (SNe). Such a mass-loss forms “confine......p> cm with the mass-loss rate of 0.01 ∼......tron radiation from the system of a red supergian...
- 参照...ermal Emission from Type Ia and Co......inal Months of Massive Star Evolution from the Circumstel......Radio Emission from Ultra-stripped Supernovae as ...
- 参照...ermal Emission from Supernova Remn......DBAND EMISSION FROM TYCHO'S SUPERN......RAY COMPONENTS FROM TYPE IIn SUPER......r Missing High-Mass Stars The Zwicky Tra......Red Supergiant Mass Loss Synchrotron Se......e of particles from cosmic ray mod......ENGTH EMISSION FROM THE VELA JR. S......nergy Emission from Interacting Su......X-ray emission from type II supern......S Constraining Massive Star Activi......r of SN 2013cu from spectral obser......X‐Ray Spectrum from Loss‐flattened Elec......ermal Emission from Circumstellar ...... ROTATION, AND MASSIVE STARS Early-time spe......ellar Emission from Type Ib and Ic Supernovae CHA...
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- 要約等...jats:p>Coronal mass ejections (CME......e star to shed mass and magnetic f......n, CME-related mass loss is roughly an ......other types of stars, CMEs have bee......away much more mass and energy tha......r use on other stars. An example pr......on of wind/CME mass-loss rates for a solar-mass star is given....... Sun), the CME mass loss exceeds that o......100 times more mass than the wind,......cumulative CME mass lost by the yo...... 1% of a solar mass.</jats:p>
- 参照... Rotator Winds from Low-mass Stars. I. Rotation D......ic Braking and Mass-loss Rate Time-reso......n and Sun-like stars
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- 参照...Nearby Evolved Stars Survey II: Con...... first results from the James Cler......earth of OH/IR stars in the Small Magellanic Cloud
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- 参照The Nearby Evolved Stars Survey II: Con...... first results from the James Clerk Maxwell Teles...
- 並列タイトル等（連結）III. Dust properties for carbon-rich asymptotic giant branch stars
- 並列タイトル等III. Dust properties for carbon-rich asymptotic giant branch stars
A Porosity‐Length Formalism for Photon‐Tiring–limited Mass Loss from Stars above the Eddington Limit
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- 並列タイトル等（連結）Mass-losing AGB stars in Sgr and Fornax
- 並列タイトル等Mass-losing AGB stars in Sgr and Fornax
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- 参照...ctive Sun-like Stars Using Solar Sc......LY DRIVEN WIND FROM GASEOUS PLANETS. II. EFFECTS ...
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- 参照The Nearby Evolved Stars Survey II: Con...... first results from the James Clerk Maxwell Teles...
- 並列タイトル等（連結）I. Theoretical model – Mass-loss history unravelled in VY CMa
- 並列タイトル等I. Theoretical model – Mass-loss history unravelled in VY CMa