中文
相关论文

相关论文: Dust as interstellar catalyst - II. How chemical d…

200 篇论文

Context. The presence of dust in the interstellar medium has profound consequences on the chemical composition of regions where stars are forming. Recent observations show that many species formed onto dust are populating the gas phase,…

太阳与恒星天体物理 · 物理学 2015-12-16 M. Minissale , F. Dulieu , S. Cazaux , S. Hocuk

Outflows of pre-main-sequence stars drive shocks into molecular material within 0.01 - 1 pc of the young stars. The shock-heated gas emits infrared, millimeter and submillimeter lines of many species including. Dust grains are important…

天体物理学 · 物理学 2010-12-13 T. W. Hartquist , S. Van Loo , S. A. E. G. Falle , P. Caselli , I. Ashmore

Dust plays an important role in the evolution of a galaxy, since it is one of the main ingredients for efficient star formation. Dust grains are also a sink/source of metals when they are created/destroyed, and, therefore, a self-consistent…

星系天体物理 · 物理学 2020-04-08 I. Millán-Irigoyen , M. Mollá , Y. Ascasibar

Molecular gas is the key ingredient of the star formation cycle, and tracing its dependencies on other galaxy properties is essential for understanding galaxy evolution. In this work, we explore the relation between the different phases of…

星系天体物理 · 物理学 2025-07-23 Francesco Salvestrini , Simone Bianchi , Edvige Corbelli

Despite its small mass fraction typically observed in the interstellar medium, dust plays a significant role as a key component of galaxies, affecting a wide range of properties. This review focuses specifically on how dust grains influence…

星系天体物理 · 物理学 2026-04-28 Francesco Calura

The evolution of star-forming regions and their thermal balance are strongly influenced by their chemical composition, that, in turn, is determined by the physico-chemical processes that govern the transition between the gas phase and the…

My thesis work aims to study the inter-relation between various physical and chemical conditions in a wide range of astrophysical environments. Our studied regions range from the super-hot regions (i.e., nebular, photon-dominated, or…

太阳与恒星天体物理 · 物理学 2022-08-12 Milan Sil

The abundances of gas and dust (solids and complex molecules) in the interstellar medium (ISM) as well as their composition and structures impact practically all of astrophysics. Fundamental processes from star formation to stellar winds to…

Stars form within dense cores composed of both gas and dust within molecular clouds. However, despite the crucial role that dust plays in the star formation process, its dynamics is frequently overlooked, with the common assumption being a…

星系天体物理 · 物理学 2025-02-21 Nadine H. Soliman , Philip F. Hopkins , Michael Y. Grudić

Context. Water together with O2 are important gas phase ingredients to cool dense gas in order to form stars. On dust grains, H2 O is an important constituent of the icy mantle in which a complex chemistry is taking place, as revealed by…

太阳与恒星天体物理 · 物理学 2015-05-19 S. Cazaux , V. Cobut , M. Marseille , M. Spaans , P. Caselli

Aims: The gas-phase abundance of methanol in dark quiescent cores in the interstellar medium cannot be explained by gas-phase chemistry. In fact, the only possible synthesis of this species appears to be production on the surfaces of dust…

天体物理学 · 物理学 2009-11-13 R. T. Garrod , V. Wakelam , E. Herbst

In molecular clouds at temperatures as low as 10 K, all species except hydrogen and helium should be locked in the heterogeneous ice on dust grain surfaces. Nevertheless, astronomical observations have detected over 150 different species in…

星系天体物理 · 物理学 2018-10-12 Y. Oba , T. Tomaru , T. Lamberts , A. Kouchi , N. Watanabe

In the interstellar medium of the Milky Way, certain elements -- e.g., Mg, Si, Al, Ca, Ti, Fe -- reside predominantly in interstellar dust grains. These grains absorb, scatter, and emit electromagnetic radiation, heat the interstellar…

天体物理学 · 物理学 2007-05-23 B. T. Draine

The past century of interstellar dust has brought us from first ignoring it to finding that it plays an important role in the evolution of galaxies. Current observational results in our galaxy provide a complex physical and chemical…

天体物理学 · 物理学 2009-10-31 J. Mayo Greenberg , Chuanjian Shen

Dust is a crucial component of the interstellar medium of galaxies. The presence of dust strongly affects the light produced by stars within a galaxy. As these photons are our main information vector to explore the stellar mass assembly and…

星系天体物理 · 物理学 2019-07-17 M. Cousin , V. Buat , G. Lagache , M. Bethermin

Ice is ubiquitous in the interstellar medium. We model the formation of the main constituents of interstellar ices, including H2O, CO2 , CO, and CH3 OH. We strive to understand what physical or chemical parameters influence the final…

星系天体物理 · 物理学 2023-07-26 A. Clément , A. Taillard , V. Wakelam , P. Gratier , J. -C. Loison , E. Dartois , F. Dulieu , J. A. Noble , M. Chabot

Chemical models have been developed over the years by astrophysicists to study the pro- cesses at play in the various environments of the interstellar medium (ISM) that define the chemical composition of the gas and the dust. These…

星系天体物理 · 物理学 2013-10-15 Marcelino Agundez , Valentine Wakelam

The evolution of the cosmic dust content and the cycle between metals and dust in the interstellar medium (ISM) play a fundamental role in galaxy evolution. The chemical enrichment of the Universe can be traced through the evolution of the…

Dust plays a key role during star, disk and planet formation. Yet, its dynamics during the protostellar collapse remains a poorly investigated field. Recent studies seem to indicate that dust may decouple efficiently from the gas during…

太阳与恒星天体物理 · 物理学 2020-09-23 Ugo Lebreuilly , Benoît Commerçon , Guillaume Laibe

The past century of interstellar dust has brought us from first ignoring it to finding that it is an important component of the interstellar medium and plays an important role in the evolution of galaxies, the formation of stars and…

天体物理学 · 物理学 2007-05-23 Aigen Li , J. Mayo Greenberg
‹ 上一页 1 2 3 10 下一页 ›