Search Results - "Bladh, Sara"

A NEW GENERATION OF PARSEC-COLIBRI STELLAR ISOCHRONES INCLUDING THE TP-AGB PHASE by Marigo, Paola, Girardi, Léo, Bressan, Alessandro, Rosenfield, Philip, Aringer, Bernhard, Chen, Yang, Dussin, Marco, Nanni, Ambra, Pastorelli, Giada, Rodrigues, Thaíse S., Trabucchi, Michele, Bladh, Sara, Dalcanton, Julianne, Groenewegen, Martin A. T., Montalbán, Josefina, Wood, Peter R.

“…We introduce a new generation of PARSEC-COLIBRI stellar isochrones that includes a detailed treatment of the thermally pulsing asymptotic giant branch (TP-AGB)…”
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Multiple Habitable Phases on Outer Exosolar Worlds by Sparrman, Viktor, Bladh, Sara, Way, M. J.

“…As stars evolve to higher luminosities during first ascension of the giant branch, previously frozen terrestrial worlds may thaw and host liquid water on their…”
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Carbon star formation as seen through the non-monotonic initial–final mass relation by Marigo, Paola, Cummings, Jeffrey D., Curtis, Jason Lee, Kalirai, Jason, Chen, Yang, Tremblay, Pier-Emmanuel, Ramirez-Ruiz, Enrico, Bergeron, Pierre, Bladh, Sara, Bressan, Alessandro, Girardi, Léo, Pastorelli, Giada, Trabucchi, Michele, Cheng, Sihao, Aringer, Bernhard, Tio, Piero Dal

“…The initial–final mass relation (IFMR) links the birth mass of a star to the mass of the compact remnant left at its death. While the relevance of the IFMR…”
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Constraining dust properties in circumstellar envelopes of C-stars in the Small Magellanic Cloud: optical constants and grain size of carbon dust by Nanni, Ambra, Marigo, Paola, Groenewegen, Martin A. T., Aringer, Bernhard, Girardi, Léo, Pastorelli, Giada, Bressan, Alessandro, Bladh, Sara

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Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Small Magellanic Cloud by Pastorelli, Giada, Marigo, Paola, Girardi, Léo, Chen, Yang, Rubele, Stefano, Trabucchi, Michele, Aringer, Bernhard, Bladh, Sara, Bressan, Alessandro, Montalbán, Josefina, Boyer, Martha L, Dalcanton, Julianne J, Eriksson, Kjell, Groenewegen, Martin A T, Höfner, Susanne, Lebzelter, Thomas, Nanni, Ambra, Rosenfield, Philip, Wood, Peter R, Cioni, Maria-Rosa L

“…Abstract The thermally pulsing asymptotic giant branch (TP-AGB) experienced by low- and intermediate-mass stars is one of the most uncertain phases of stellar…”
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Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud by Pastorelli, Giada, Marigo, Paola, Girardi, Léo, Aringer, Bernhard, Chen, Yang, Rubele, Stefano, Trabucchi, Michele, Bladh, Sara, Boyer, Martha L, Bressan, Alessandro, Dalcanton, Julianne J, Groenewegen, Martin A T, Lebzelter, Thomas, Mowlavi, Nami, Chubb, Katy L, Cioni, Maria-Rosa L, de Grijs, Richard, Ivanov, Valentin D, Nanni, Ambra, van Loon, Jacco Th, Zaggia, Simone

“…ABSTRACT Reliable models of the thermally pulsing asymptotic giant branch (TP-AGB) phase are of critical importance across astrophysics, including our…”
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Constraining dust properties in circumstellar envelopes of C-stars in the Small Magellanic Cloud: optical constants and grain size of carbon dust by Nanni, Ambra, Marigo, Paola, Groenewegen, Martin A. T., Aringer, Bernhard, Girardi, Léo, Pastorelli, Giada, Bressan, Alessandro, Bladh, Sara

“…We present a new approach aimed at constraining the typical size and optical properties of carbon dust grains in circumstellar envelopes (CSEs) of carbon-rich…”
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The evolution of DARWIN: current status of wind models for AGB stars by Bladh, Sara

“…A&A 626, A100 (2019) The slow, dense winds observed in evolved asymptotic giant branch (AGB) stars are usually attributed to a combination of dust formation in…”
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Dynamic atmospheres and winds of cool luminous giants, II. Gradual Fe enrichment of wind-driving silicate grains by Höfner, Susanne, Bladh, Sara, Aringer, Bernhard, Eriksson, Kjell

“…A&A 657, A109 (2022) The winds observed around AGB stars are generally attributed to radiation pressure on dust formed in the dynamical atmospheres of these…”
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Modelling polarized light from dust shells surrounding asymptotic giant branch stars by Aronson, Erik, Bladh, Sara, Höfner, Susanne

“…A&A 603, A116 (2017) Winds of asymptotic giant branch (AGB) stars are commonly assumed to be driven by radiative acceleration of dust grains. For M-type AGB…”
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Exploring wind-driving dust species in cool luminous giants I. Basic criteria and dynamical models of M-type AGB stars by Bladh, Sara, Höfner, Susanne

“…A&A (2012), 546, A76 This work is part of an ongoing effort aiming at identifying the actual wind-drivers among the dust species observed in circumstellar…”
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Dynamic atmospheres and winds of cool luminous giants, I. Al$_2$O$_3$ and silicate dust in the close vicinity of M-type AGB stars by Höfner, Susanne, Bladh, Sara, Aringer, Bernhard, Ahuja, Rajeev

“…A&A 594, A108 (2016) High spatial resolution techniques have given valuable insights into the mass loss mechanism of AGB stars, which presumably involves a…”
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Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud by Pastorelli, Giada, Marigo, Paola, Girardi, Léo, Aringer, Bernhard, Chen, Yang, Rubele, Stefano, Trabucchi, Michele, Bladh, Sara, Boyer, Martha L, Bressan, Alessandro, Dalcanton, Julianne J, Groenewegen, Martin A. T, Lebzelter, Thomas, Mowlavi, Nami, Chubb, Katy L, Cioni, Maria-Rosa L, de Grijs, Richard, Ivanov, Valentin D, Nanni, Ambra, van Loon, Jacco Th, Zaggia, Simone

“…Reliable models of the thermally pulsing asymptotic giant branch (TP-AGB) phase are of critical importance across astrophysics, including our interpretation of…”
Get full text

Carbon star formation as seen through the non-monotonic initial-final mass relation by Marigo, Paola, Cummings, Jeffrey D, Curtis, Jason Lee, Kalirai, Jason, Chen, Yang, Tremblay, Pier-Emmanuel, Ramirez-Ruiz, Enrico, Bergeron, Pierre, Bladh, Sara, Bressan, Alessandro, Girardi, Leo, Pastorelli, Giada, Trabucchi, Michele, Cheng, Sihao, Aringer, Bernhard, Tio, Piero Dal

“…The initial-final mass relation (IFMR) links the birth mass of a star to the mass of the compact remnant left at its death. While the relevance of the IFMR…”
Get full text

Constraining the thermally-pulsing asymptotic giant branch phase with resolved stellar populations in the Small Magellanic Cloud by Pastorelli, Giada, Marigo, Paola, Girardi, Léo, Chen, Yang, Rubele, Stefano, Trabucchi, Michele, Aringer, Bernhard, Bladh, Sara, Bressan, Alessandro, Montalbán, Josefina, Boyer, Martha L, Dalcanton, Julianne J, Eriksson, Kjell, Groenewegen, Martin A. T, Höfner, Susanne, Lebzelter, Thomas, Nanni, Ambra, Rosenfield, Philip, Wood, Peter R, Cioni, Maria-Rosa L

“…The thermally-pulsing asymptotic giant branch (TP-AGB) experienced by low- and intermediate-mass stars is one of the most uncertain phases of stellar evolution…”
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Cool, evolved stars: results, challenges, and promises for the next decade by Rau, Gioia, MontezJr, Rodolfo, Carpenter, Kenneth G, Wittkowski, Markus, Bladh, Sara, Karovska, Margarita, Airapetian, Vladimir, Ayres, Tom, Boyer, Martha, Chiavassa, Andrea, Clayton, Geoffrey, Danchi, William, De Marco, Orsola, Dupree, Andrea K, Kaminski, Tomasz, Kastner, Joel H, Kerschbaum, Franz, Linsky, Jeffrey, Lopez, Bruno, Monnier, John, Montargès, Miguel, Nielsen, Krister, Ohnaka, Keiichi, Ramstedt, Sofia, Roettenbacher, Rachael, Brummelaar, Theo ten, Paladini, C, Sarangi, Arkaprabha, van Belle, Gerard, Ventura, Paolo

“…Cool, evolved stars are the main source of chemical enrichment of the interstellar medium (ISM), and understanding their mass loss and structure offers a…”
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Exploring wind-driving dust species in cool luminous giants II. Constraints from photometry of M-type AGB stars by Bladh, Sara, Höfner, Susanne, Nowotny, Walter, Aringer, Bernhard

“…The heavy mass loss observed in evolved asymptotic giant branch (AGB) stars is usually attributed to a two-stage process: atmospheric levitation by…”
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Dust in AGB stars: transparent or opaque? by Bladh, Sara, Höfner, Susanne, Aringer, Bernhard

“…It is commonly believed that winds of cool giants in their late evolutionary stages are driven by radiative pressure on dust grains, but the actual grain…”
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Constraining dust properties in Circumstellar Envelopes of C-stars in the Small Magellanic Cloud: optical constants and grain size of Carbon dust by Nanni, Ambra, Marigo, Paola, Groenewegen, Martin A. T, Aringer, Bernhard, Girardi, Léo, Pastorelli, Giada, Bressan, Alessandro, Bladh, Sara

“…We present a new approach aimed at constraining the typical size and optical properties of carbon dust grains in Circumstellar envelopes (CSEs) of carbon-rich…”
Get full text

A new generation of PARSEC-COLIBRI stellar isochrones including the TP-AGB phase by Marigo, Paola, Girardi, Leo, Bressan, Alessandro, Rosenfield, Philip, Aringer, Bernhard, Chen, Yang, Dussin, Marco, Nanni, Ambra, Pastorelli, Giada, Rodrigues, Thaise S, Trabucchi, Michele, Bladh, Sara, Dalcanton, Julianne, Groenewegen, Martin A. T, Montalban, Josefina, Wood, Peter R

“…The Astrophysical Journal 835, 77 (2017) We introduce a new generation of PARSEC-COLIBRI stellar isochrones that include a detailed treatment of the…”
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