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  1. 401
    “…In multiple stellar systems, interactions among the companion stars and their discs affect planet formation. …”
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    Dust dynamics in planet-forming discs in binary systems
  2. 402
    “…Ideas on the early stages of stellar formation and on the stellar initial mass function have been clarified. …”
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    ISO Science Legacy: A Compact Review of ISO Major Achievements
  3. 403
    por Elia, Davide, Molinari, S., Schisano, E., Pestalozzi, M., Pezzuto, S., Merello, M., Noriega-Crespo, A., Moore, T.J. T., Russeil, D., Mottram, J.C., Paladini, R., Strafella, F., Benedettini, M., Bernard, J.P., Di Giorgio, A., Eden, D.J., Fukui, Y., Plume, R., Bally, J., Martin, P.G., Ragan, S.E., Jaffa, S.E., Motte, F., Olmi, L., Schneider, N., Testi, L., Wyrowski, F., Zavagno, A., Calzoletti, L., Faustini, F., Natoli, P., Palmeirim, P., Piacentini, F., Piazzo, L., Pilbratt, G.L., Polychroni, D., Baldeschi, A., Beltran, M.T., Billot, N., Cambresy, L., Cesaroni, R., García-Lario, P., Hoare, M.G., Huang, M., Joncas, G., Liu, S.J., Maiolo, B.M. T., Marsh, K.A., Maruccia, Y., Mege, P., Peretto, N., Rygl, K.L. J., Schilke, P., Thompson, M.A., Traficante, A., Umana, G., Veneziani, M., Ward-Thompson, D., Whitworth, A.P., Arab, H., Bandieramonte, M., Becciani, U., Brescia, M., Buemi, C., Bufano, F., Butora, R., Cavuoti, S., Costa, A., Fiorellino, E., Hajnal, A., Hayakawa, T., Kacsuk, P., Leto, P., Causi, G. Li, Marchili, N., Martinavarro-Armengol, S., Mercurio, A., Molinaro, M., Riccio, G., Sano, H., Sciacca, E., Tachihara, K., Torii, K., Trigilio, C., Vitello, F., Yamamoto, H.
    Publicado 2017
    “…We also explore evolutionary status metrics such as the dust temperature, luminosity and bolometric temperature, finding that these are higher in protostellar sources compared to pre-stellar ones. The surface density of sources follows an increasing trend as they evolve from pre-stellar to protostellar, but then it is found to decrease again in the majority of the most evolved clumps. …”
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    The Hi-GAL compact source catalogue – I. The physical properties of the clumps in the inner Galaxy (−71$_{.}^{\circ}$0 < ℓ < 67$_{.}^{\circ}$0)
  4. 404
    “…Spectropolarimetric data allow for simultaneous monitoring of stellar chromospheric logR′HK activity and the surface-averaged longitudinal magnetic field, , giving the opportunity to probe the relationship between large-scale stellar magnetic fields and chromospheric manifestations of magnetism. …”
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    Linking chromospheric activity and magnetic field properties for late-type dwarf stars
  5. 405
    “…We search for the gravitational imprint of an ULDM soliton on stellar orbits near Sgr A* and by combining stellar velocity measurements with Event Horizon Telescope imaging of M87*. …”
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    Looking for ultralight dark matter near supermassive black holes
  6. 406
    “…We suggest that “<math display="inline"><mi>G</mi></math> objects” recently discovered in the Galactic Center may be clouds of gas bound by the gravitational field of stellar-mass black holes produced in the interactions of sublunar primordial black holes with neutron stars. …”
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    <math display="inline"><mi>G</mi></math> objects and primordial black holes
  7. 407
    por von Braun, Kaspar, Boyajian, Tabetha
    Publicado 2017
    “…Planetary parameters are often directly dependent upon their stellar counterparts. In addition, the star is almost always the only visible component of the system and contains most of the system mass. …”
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    Extrasolar planets and their host stars
  8. 408
    por Beech, Martin
    Publicado 2019
    “…This textbook introduces the reader to the basic concepts and equations that describe stellar structure. Various approximation techniques are used to solve equations, and an intuitive rather than rigorous approach is employed to interpret the properties of the stars. …”
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    Introducing the stars: formation, structure and evolution
  9. 409
    por Lederer-Woods, C, Woods, P J, Davinson, T, Estrade, A, Heyse, J, Kahl, D, Lonsdale, S J, Paradela, C, Schillebeeckx, P, Aberle, O, Amaducci, S, Andrzejewski, J, Audouin, L, Bacak, M, Balibrea, J, Barbagallo, M, Bečvář, F, Berthoumieux, E, Billowes, J, Bosnar, D, Brown, A, Caamaño, M, Calviño, F, Calviani, M, Cano-Ott, D, Cardella, R, Casanovas, A, Cerutti, F, Chen, Y H, Chiaveri, E, Colonna, N, Cortés, G, Cortés-Giraldo, M A, Cosentino, L, Cristallo, S, Damone, L A, Diakaki, M, Domingo-Pardo, C, Dressler, R, Dupont, E, Durán, I, Fernández-Domínguez, B, Ferrari, A, Ferreira, P, Ferrer, F J, Finocchiaro, P, Furman, V, Göbel, K, García, A R, Gawlik, A, Gilardoni, S, Glodariu, T, Gonçalves, I F, González-Romero, E, Griesmayer, E, Guerrero, C, Gunsing, F, Harada, H, Heinitz, S, Jenkins, D G, Jericha, E, Käppeler, F, Kadi, Y, Kalamara, A, Kavrigin, P, Kimura, A, Kivel, N, Kokkoris, M, Krtička, M, Kurtulgil, D, Leal-Cidoncha, E, Leeb, H, Lerendegui-Marco, J, Lo Meo, S, Macina, D, Manna, A, Marganiec, J, Martínez, T, Masi, A, Massimi, C, Mastinu, P, Mastromarco, M, Maugeri, E A, Mazzone, A, Mendoza, E, Mengoni, A, Milazzo, P M, Mingrone, F, Musumarra, A, Negret, A, Nolte, R, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Porras, I, Praena, J, Quesada, J M, Radeck, D, Rauscher, T, Reifarth, R, Rubbia, C, Ryan, J A, Sabaté-Gilarte, M, Saxena, A, Schumann, D, Sedyshev, P, Smith, A G, Sosnin, N V, Stamatopoulos, A, Tagliente, G, Tain, J L, Tarifeño-Saldivia, A, Tassan-Got, L, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vlachoudis, V, Vlastou, R, Wallner, A, Warren, S, Weiss, C, Wright, T, Žugec, P
    Publicado 2021
    “…We use our data to calculate astrophysical reactivities for stellar temperatures up to 0.7 GK. Our results resolve a discrepancy between the two previous direct measurements of this reaction, and indicate higher stellar destruction rates than the most recently recommended reactivity.…”
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    Destruction of the cosmic γ-ray emitter $^{26}$Al in massive stars: Study of the key $^{26}$Al$(n,\alpha)$ reaction
  10. 410
    por CERN. Geneva
    Publicado 2001
    “…We show that outside a narrow window of 0.5% of the strength or range of the strong interaction the stellar production of carbon or oxygen is reduced by factors of 130 to 1000. …”
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    Fine Tuning of Basic Forces through the Existence of Carbon-Based Life
  11. 411
    “…Stars may not accumulate their mass steadily, as was previously thought, but in a series of violent events manifesting themselves as sharp stellar brightening. These events can be caused by fragmentation due to gravitational instabilities in massive gaseous disks surrounding young stars, followed by migration of dense gaseous clumps onto the star. …”
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    Circumstellar disks of the most vigorously accreting young stars
  12. 412
    por Thomas, John H, Weiss, Nigel O
    Publicado 2008
    “…A comprehensive account of sunspots and starspots for graduate students, astronomers, geophysicists, space physicists and experts in solar and stellar physics.…”
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    Sunspots and starspots
  13. 413
    por Mastromarco, M, Mazzone, A, Massimi, C, Cristallo, S, Colonna, N, Aberle, O, Alcayne, V, Amaducci, S, Andrzejewski, J, Audouin, L, Babiano-Suarez, V, Bacak, M, Barbagallo, M, Bennett, S, Berthoumieux, E, Bosnar, D, Brown, A S, Busso, M, Caamaño, M, Caballero, L, Calviani, M, Calviño, F, Cano-Ott, D, Casanovas, A, Cerutti, F, Chiaveri, E, Cortés, G P, Cortés-Giraldo, M A, Cosentino, L, Damone, L A, Davies, P J, Diakaki, M, Dietz, M, Domingo-Pardo, C, Dressler, R, Ducasse, Q, Dupont, E, Durán, I, Eleme, Z, Fernández-Domíngez, B, Ferrari, A, Ferro-Gonçalves, I, Finocchiaro, P, Furman, V, Garg, R, Gawlik, A, Gilardoni, S, Göbel, K, González-Romero, E, Guerrero, C, Gunsing, F, Heinitz, S, Heyse, J, Jenkins, D G, Jericha, E, Jiri, U, Junghans, A, Kadi, Y, Käppeler, F, Kimura, A, Knapová, I, Kokkoris, M, Kopatch, Y, Krtička, M, Kurtulgil, D, Ladarescu, I, Lederer-Woods, C, Lerendegui-Marco, J, Lonsdale, S -J, Macina, D, Manna, A, Martínez, T, Masi, A, Mastinu, P F, Maugeri, E, Mendoza, E, Mengoni, A, Michalopoulou, V, Milazzo, P M, Millán-Callado, M A, Mingrone, F, Moreno-Soto, J, Musumarra, A, Negret, A, Ogállar, F, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Petrone, C, Piersanti, L, Pirovano, E, Porras, I, Praena, J, Quesada, J M, Ramos Doval, D, Reifarth, R, Rochman, D, Rubbia, C, Sabaté-Gilarte, M, Saxena, A, Schillebeeckx, P, Schumann, D, Sekhar, A, Smith, A G, Sosnin, N, Sprung, P, Stamatopoulos, A, Tagliente, G, Tain, J L, Tarifeño-Saldivia, A E, Tassan-Got, L, Thomas, B, Torres-Sánchez, P, Tsinganis, A, Urlass, S, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vescovi, D, Vlachoudis, V, Vlastou, R, Wallner, A, Woods, P J, Wright, T J, Žugec, P
    Publicado 2020
    “…Such a quasi pure s-process origin makes them crucial for testing the robustness of stellar models in galactic chemical evolution (GCE). …”
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    The $^{154}$Gd neutron capture cross section measured at the n_TOF facility and its astrophysical implications
  14. 414
    “…A wide range of topics is covered, from stellar and nebular astrophysics to galactic dynamics and galaxy clusters, making this volume a unique and timely reference of broad astrophysical interest.…”
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    Planetary Nebulae Beyond the Milky Way
  15. 415
    “…The book also offers an introductory chapter on stellar evolution written by the editors of the book.…”
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    Ecology of blue straggler stars
  16. 416
    por Sosnin, N V, Lederer-Woods, C, Krtička, M, Garg, R, Dietz, M, Bacak, M, Barbagallo, M, Battino, U, Cristallo, S, Damone, L A, Diakaki, M, Heinitz, S, Macina, D, Mastromarco, M, Mingrone, F, St J Murphy, A, Tagliente, G, Valenta, S, Vescovi, D, Aberle, O, Alcayne, V, Amaducci, S, Andrzejewski, J, Audouin, L, Bécares, V, Babiano-Suarez, V, Bečvář, F, Bellia, G, Berthoumieux, E, Billowes, J, Bosnar, D, Brown, A, Busso, M, Caamaño, M, Caballero, L, Calviño, F, Calviani, M, Cano-Ott, D, Casanovas, A, Cerutti, F, Chen, Y H, Chiaveri, E, Colonna, N, Cortés, G, Cortés-Giraldo, M A, Cosentino, L, Domingo-Pardo, C, Dressler, R, Dupont, E, Durán, I, Eleme, Z, Fernández-Domínguez, B, Ferrari, A, Finocchiaro, P, Göbel, K, Gawlik-Ramięga, A, Gilardoni, S, Glodariu, T, Gonçalves, I F, González-Romero, E, Guerrero, C, Gunsing, F, Harada, H, Heyse, J, Jenkins, D G, Jericha, E, Käppeler, F, Kadi, Y, Kimura, A, Kivel, N, Kokkoris, M, Kurtulgil, D, Ladarescu, I, Leeb, H, Lerendegui-Marco, J, Meo, S Lo, Lonsdale, S J, Manna, A, Martínez, T, Masi, A, Massimi, C, Mastinu, P, Matteucci, F, Maugeri, E A, Mazzone, A, Mendoza, E, Mengoni, A, Michalopoulou, V, Milazzo, P M, Musumarra, A, Negret, A, Nolte, R, Ogállar, F, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Piersanti, L, Porras, I, Praena, J, Quesada, J M, Radeck, D, Ramos-Doval, D, Rauscher, T, Reifarth, R, Rochman, D, Rubbia, C, Sabaté-Gilarte, M, Saxena, A, Schillebeeckx, P, Schumann, D, Smith, A G, Stamatopoulos, A, Tain, J L, Talip, T, Tarifeño-Saldivia, A, Tassan-Got, L, Torres-Sánchez, P, Tsinganis, A, Ulrich, J, Urlass, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vlachoudis, V, Vlastou, R, Wallner, A, Woods, P J, Wright, T, Žugec, P
    Publicado 2023
    “…Maxwellian-averaged cross sections were calculated for stellar temperatures between kT=5keV and kT=100keV, with uncertainties between 4.2% and 5.7%. …”
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    Measurement of the Se77(n,γ) cross section up to 200 keV at the n_TOF facility at CERN
  17. 417
    “…As all four events can reasonably be attributed to stellar lenses, we conclude that our subsample of high ratio signal-to-noise candidates does not require the presence of MACHOs.…”
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    The Point-Agape survey: No Need for Machos in M31 ?
  18. 418
    “…We show that paradoxically, although metal-rich stars emit substantially less ultraviolet radiation than metal-poor stars, the surface of their planets is exposed to more intense ultraviolet radiation. For the stellar types considered, metallicity has a larger impact than stellar temperature. …”
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    Metal-rich stars are less suitable for the evolution of life on their planets
  19. 419
    por Fryer, Chris L., New, Kimberly C. B.
    Publicado 2003
    “…Gravitational wave emission from stellar collapse has been studied for more than three decades. …”
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    Gravitational Waves from Gravitational Collapse
  20. 420
    por Fryer, Chris L., New, Kimberly C. B.
    Publicado 2011
    “…Gravitational-wave emission from stellar collapse has been studied for nearly four decades. …”
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    Gravitational Waves from Gravitational Collapse
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