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We analyze thermal emission of radiation in homogeneous clouds. The clouds have negligible horizontal variation, but the temperature can vary vertically. The radiation at optical depth $\tau$ above the cloud bottom is characterized by…

大气与海洋物理 · 物理学 2023-01-20 W. A. van Wijngaarden , W. Happer

The first complete far-infrared spectrum of T Tau has been obtained with the LWS spectrometer on-board the Infrared Space Observatory, which detected strong emission from high-J (J=14-25) CO, para- and ortho-H2O and OH transitions over the…

We investigate the optical linear polarization caused by Thomson scattering of the stellar radiation for gamma-ray binary \lsi61, which likely contains a young pulsar. Based on the pulsar binary scenario, we model the interaction between…

高能天体物理现象 · 物理学 2025-10-14 Jiaxin Liu , Haoyu Yuan , Xiangli Lei , Wenlong Xu , Jumpei Takata , Weihua Lei

(Abridged) We use high S/N spectra of 20 HII regions in the giant spiral galaxy M101 to derive electron temperatures for the HII regions and robust metal abundances over radii R = 0.19-1.25 Ro (6-41 kpc). We compare the consistency of…

天体物理学 · 物理学 2009-11-07 Robert C. Kennicutt , Fabio Bresolin , Don R. Garnett

Very high energy resolution photoemission experiments on high quality samples of optimally doped Bi$_2$Sr$_2$CaCu$_2$O$_{8+\delta}$ show new features in the low-energy electronic excitations. A marked change in the binding energy and…

超导电性 · 物理学 2007-05-23 T. Valla , T. E. Kidd , J. D. Rameau , H. -J. Noh , G. D. Gu , P. D. Johnson , H. -B. Yang , H. Ding

X-rays/EUV radiation emitted from wind-embedded shocks in hot, massive stars can affect the ionization balance in their outer atmospheres, and can be the mechanism responsible for the production of highly ionized species. To allow for these…

太阳与恒星天体物理 · 物理学 2016-05-18 Luiz P. Carneiro , J. Puls , J. O. Sundqvist , T. L. Hoffmann

We investigate the escape of Ly$\beta$ from emission nebulae with a significant population of excited hydrogen atoms in the level $n=2$, rendering them optically thick in H$\alpha$. The transfer of Ly$\beta$ line photons in these optically…

高能天体物理现象 · 物理学 2018-03-21 Seok-Jun Chang , Hee-Won Lee , Sang-Hyeon Ahn , Hogyu Lee , Rodolfo Angeloni , Tali Palma , Francesco Di Mille

SBS 0335$-$052 E is an extremely low-metallicity ($Z\sim0.04\,Z_{\odot}$) blue compact dwarf galaxy. An active galactic nucleus has been proposed to explain the broad H$\alpha$ emission and near-infrared (NIR) time variability in super star…

We report measurements of the electron temperature at about a dozen locations in the extended emission-line regions of five active (Seyfert and radio) galaxies. Temperatures (T_{[OIII]} and T_{[NII]}) have been determined from both the…

天体物理学 · 物理学 2016-08-30 A. S. Wilson , L. Binette , T. Storchi-Bergmann

We show that the line broadening in quiescent solar prominences is mainly due to non-thermal velocities. We have simultaneously observed a wide range of optically thin lines in quiescent prominences, selected for bright and narrow Mg\,b…

太阳与恒星天体物理 · 物理学 2016-05-26 Goetz Stellmacher , Eberhard Wiehr

The low-temperature behavior of the electron phase coherence time, $\tau_{\phi}$, in mesoscopic metal wires has been a subject of controversy recently. Whereas theory predicts that $\tau_{\phi}(T)$ in narrow wires should increase as…

介观与纳米尺度物理 · 物理学 2015-06-24 Norman O. Birge , F. Pierre

A recently generated theoretical line list of C II dielectronic recombination lines together with observational data gathered from the literature is used to investigate the electron temperature in a range of astronomical objects, mainly…

太阳与恒星天体物理 · 物理学 2013-01-16 Peter J. Storey , Taha Sochi

Measurements of the ratio of the proton elastic form factors ($\mu_pG_E/G_M$) using Rosenbluth separation and those using polarization-based techniques show a strong discrepancy, which increases as a function of $Q^2$. The contribution of…

核实验 · 物理学 2017-12-07 Brian S. Henderson

Bow shocks and related density enhancements produced by the winds of massive stars moving through the interstellar medium provide important information regarding the motions of the stars, the properties of their stellar winds, and the…

太阳与恒星天体物理 · 物理学 2018-04-04 Manisha Shrestha , Hilding R. Neilson , Jennifer L. Hoffman , Richard Ignace

The spatial structure of the emission lines and continuum over the 50 arcsecond extent of the nearby, O-rich, planetary nebula NGC 7009 (Saturn Nebula) have been observed with the MUSE integral field spectrograph on the ESO Very Large…

We detect near-infrared H2 emission in DG Tau using the Infrared Camera and Spectrograph (IRCS) on the 8.2-m SUBARU telescope. The spectra obtained along the jet axis show that the centroidal position of the 1-0 S(1) emission is offset by…

天体物理学 · 物理学 2009-11-10 M. Takami , A. Chrysostomou , T. P. Ray , C. Davis , W. R. F. Dent , J. Bailey , M. Tamura , H. Terada

We study X-ray and soft gamma-ray spectra from the hard state of the accreting black-hole binary MAXI J1820+070. We perform analysis of two joint spectra from NuSTAR and INTEGRAL, covering the range of 3--650 keV, and of an average joint…

we identify the intrinsic bulk pairing symmetry for both electron and hole-doped cuprates from the existing bulk- and nearly bulk-sensitive experimental results such as magnetic penetration depth, Raman scattering, single-particle…

超导电性 · 物理学 2009-11-07 Guo-meng Zhao

We present radio observations (1--40 GHz) for 36 classical novae, representing data from over five decades compiled from the literature, telescope archives, and our own programs. Our targets display a striking diversity in their optical…

The temperature dependence of the complex optical properties of the layered phosphide material EuCd$_2$P$_2$ have been measured over a wide frequency range above and below $T_{\rm N} \simeq 11.5$ K for light polarized in the $a-b$ planes.…

强关联电子 · 物理学 2023-03-23 C. C. Homes , Z. -C. Wang , K. Fruhling , F. Tafti