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zadetkov: 921
1.
  • 2D wind clumping in hot, ma... 2D wind clumping in hot, massive stars from hydrodynamical line-driven instability simulations using a pseudo-planar approach
    Sundqvist, J. O.; Owocki, S. P.; Puls, J. Astronomy and astrophysics (Berlin), 03/2018, Letnik: 611
    Journal Article
    Recenzirano
    Odprti dostop

    Context. Clumping in the radiation-driven winds of hot, massive stars arises naturally due to the strong, intrinsic instability of line-driving (the line-deshadowing instability, hereafter LDI). But ...
Celotno besedilo
Dostopno za: FMFMET, NUK, UL, UM, UPUK

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2.
  • An excess of massive stars ... An excess of massive stars in the local 30 Doradus starburst
    Schneider, F R N; Sana, H; Evans, C J ... Science (American Association for the Advancement of Science), 01/2018, Letnik: 359, Številka: 6371
    Journal Article
    Recenzirano
    Odprti dostop

    The 30 Doradus star-forming region in the Large Magellanic Cloud is a nearby analog of large star-formation events in the distant universe. We determined the recent formation history and the initial ...
Celotno besedilo
Dostopno za: BFBNIB, NMLJ, NUK, ODKLJ, PNG, SAZU, UL, UM, UPUK

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3.
  • Ephemeris, orbital decay, a... Ephemeris, orbital decay, and masses of ten eclipsing high-mass X-ray binaries
    Falanga, M.; Bozzo, E.; Lutovinov, A. ... Astronomy and astrophysics (Berlin), 05/2015, Letnik: 577
    Journal Article
    Recenzirano
    Odprti dostop

    We update the ephemeris of the eclipsing high-mass X-ray binary (HMXB) systems LMC X-4, Cen X-3, 4U 1700-377, 4U 1538-522, SMC X-1, IGR J18027-2016, Vela X-1,IGR J17252-3616, XTE J1855-026, and OAO ...
Celotno besedilo
Dostopno za: FMFMET, NUK, UL, UM, UPUK

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4.
  • 3D collagen fibrillar micro... 3D collagen fibrillar microstructure guides pancreatic cancer cell phenotype and serves as a critical design parameter for phenotypic models of EMT
    Puls, T J; Tan, Xiaohong; Whittington, Catherine F ... PloS one, 11/2017, Letnik: 12, Številka: 11
    Journal Article
    Recenzirano
    Odprti dostop

    Pancreatic cancer, one of the deadliest cancers, is characterized by high rates of metastasis and intense desmoplasia, both of which are associated with changes in fibrillar type I collagen ...
Celotno besedilo
Dostopno za: DOBA, IZUM, KILJ, NUK, PILJ, PNG, SAZU, SIK, UILJ, UKNU, UL, UM, UPUK

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5.
  • Mass loss from inhomogeneou... Mass loss from inhomogeneous hot star winds
    Sundqvist, J O; Puls, J; Owocki, S P Astronomy and astrophysics (Berlin), 08/2014, Letnik: 568
    Journal Article
    Recenzirano
    Odprti dostop

    We provide a fast and easy-to-use formalism for treating the reduction in effective opacity associated with optically thick clumps in an accelerating two-component medium. This study shows that ...
Celotno besedilo
Dostopno za: FMFMET, NUK, UL, UM, UPUK

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6.
  • The IACOB project The IACOB project
    Simon-Diaz, S; Godart, M; Castro, N ... Astronomy and astrophysics (Berlin), 1/2017, Letnik: 597
    Journal Article, Web Resource
    Recenzirano
    Odprti dostop

    Context. The term macroturbulent broadening is commonly used to refer to a certain type of non-rotational broadening affecting the spectral line profiles of O- and B-type stars. It has been proposed ...
Celotno besedilo
Dostopno za: FMFMET, NUK, UL, UM, UPUK

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7.
  • To clump or not to clump To clump or not to clump
    Rübke, K; Herrero, A; Puls, J Astronomy and astrophysics (Berlin), 11/2023, Letnik: 679
    Journal Article
    Recenzirano
    Odprti dostop

    Context. Winds of massive stars have density inhomogeneities (clumping) that may affect the formation of spectral lines in different ways, depending on their formation region. Most of previous and ...
Celotno besedilo
Dostopno za: FMFMET, NUK, UL, UM, UPUK
8.
  • L-band spectroscopy of Gala... L-band spectroscopy of Galactic OB-stars
    Najarro, F.; Hanson, M. M.; Puls, J. Astronomy and astrophysics (Berlin), 11/2011, Letnik: 535
    Journal Article
    Recenzirano
    Odprti dostop

    Context. Mass-loss, occurring through radiation driven supersonic winds, is a key issue throughout the evolution of massive stars. Two outstanding problems are currently challenging the theory of ...
Celotno besedilo
Dostopno za: FMFMET, NUK, UL, UM, UPUK

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9.
  • 3D radiative transfer: Cont... 3D radiative transfer: Continuum and line scattering in non-spherical winds from OB stars
    Hennicker, L.; Puls, J.; Kee, N. D. ... Astronomy and astrophysics (Berlin), 08/2018, Letnik: 616
    Journal Article
    Recenzirano
    Odprti dostop

    Context. State of the art quantitative spectroscopy utilizes synthetic spectra to extract information from observations. For hot, massive stars, these synthetic spectra are calculated by means of 1D, ...
Celotno besedilo
Dostopno za: FMFMET, NUK, UL, UM, UPUK

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10.
  • A 3D short-characteristics ... A 3D short-characteristics method for continuum and line scattering problems in the winds of hot stars
    Hennicker, L.; Puls, J.; Kee, N. D. ... Astronomy and astrophysics (Berlin), 01/2020, Letnik: 633
    Journal Article
    Recenzirano
    Odprti dostop

    Context. Knowledge about hot, massive stars is usually inferred from quantitative spectroscopy. To analyse non-spherical phenomena, the existing 1D codes must be extended to higher dimensions, and ...
Celotno besedilo
Dostopno za: FMFMET, NUK, UL, UM, UPUK

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zadetkov: 921

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