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相关论文: New upper limits on the interstellar O2 abundance

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Recent observations of high redshift quasars at z~6 have finally revealed complete Gunn-Peterson absorption. However, this at best constrains the volume-weighted and mass-weighted hydrogen neutral fractions to be greater than 10^-3 and…

天体物理学 · 物理学 2009-11-07 S. Peng Oh

We report on a survey for associated HI 21-cm and OH 18-cm absorption with the Giant Metrewave Radio Telescope at redshifts z = 0.2-0.4. Although the low redshift selection ensures that our targets are below the critical ultra-violet…

星系天体物理 · 物理学 2017-03-29 S. J. Curran , M. T. Whiting , J. R. Allison , A. Tanna E. M. Sadler , R. Athreya

The nature of the Local Interstellar Cloud (LIC) is highly constrained by the combination of in situ heliospheric and line-of-sight data towards nearby stars. We present a new interpretation of the LIC components of the absorption line data…

天体物理学 · 物理学 2011-02-11 Jonathan D. Slavin , Priscilla C. Frisch

We present 92cm observations of the high-redshift galaxy B2 0902+343 (z=3.40) with the Westerbork Synthesis Radio Telescope (WSRT). Twenty-one cm HI is detected in absorption, at a depth of 15.9 mJy (=~6\sigma) and rest frame velocity width…

天体物理学 · 物理学 2009-11-07 Ann Marie Cody , Robert Braun

We have searched for molecular absorption lines at millimeter wavelengths in eleven gravitational lens systems discovered in the JVAS/CLASS surveys of flat spectrum radio sources. Spectra of only one source 1030+074 were obtained in the 3-,…

天体物理学 · 物理学 2009-10-31 E. Xanthopoulos , F. Combes , T. Wiklind

We present the methodology for ``blind'' millimetre-wave surveys for redshifted molecular absorption in the CO/HCO$^+$ rotational lines. The frequency range $30-50$ GHz appears optimal for such surveys, providing sensitivity to absorbers at…

星系天体物理 · 物理学 2014-06-19 N. Kanekar , A. Gupta , C. L. Carilli , J. T. Stocke , K. W. Willett

Using the Effelsberg 100-m telescope, absorption in the (J,K) = (1,1), (2,2) and (3,3) inversion lines of ammonia (NH_3) was detected at a redshift of z = 0.6847 toward the gravitational lens system B0218+357. The lambda ~ 2cm absorption…

天体物理学 · 物理学 2009-11-11 C. Henkel , N. Jethava , A. Kraus , K. M. Menten , C. L. Carilli , M. Grasshoff , D. Lubowich , M. J. Reid , .

We present an analysis of interstellar absorption lines in high-resolution optical echelle spectra of SS Cyg obtained during an outburst in 2013 June and in archival Hubble Space Telescope and Far Ultraviolet Spectroscopic Explorer data.…

星系天体物理 · 物理学 2018-06-07 Adam M. Ritchey , George Wallerstein , Jean McKeever

Hyperfine structure lines of highly-charged ions may open a new window in observations of hot rarefied astrophysical plasmas. In this paper we discuss spectral lines of isotopes and ions abundant at temperatures 10^5-10^7 K, characteristic…

天体物理学 · 物理学 2010-11-11 R. A. Sunyaev , D. Docenko

The understanding of interstellar nitrogen chemistry has improved significantly with recent results from the Herschel Space Observatory. To set even better constraints, we report here on deep searches for the NH+ ground state rotational…

We report on the detection of atomic oxygen lines in the spectra of 8 comets. These forbidden lines are a result of the photodissociation of the parent oxygen-bearing species directly into an excited state. We used high resolution spectra…

天体物理学 · 物理学 2009-11-13 Anita L. Cochran

The low-redshift Ly-alpha forest of absorption lines provides a probe of large-scale baryonic structures in the intergalactic medium, some of which may be remnants of physical conditions set up during the epoch of galaxy formation. We…

天体物理学 · 物理学 2019-08-17 J. Michael Shull , Steven V. Penton , John T. Stocke

I present the first molecular line survey of the strongly lensed submillimetre galaxy SPT-S J002706-5007.4 ($z = 3.44$) using the new Atacama Large Millimeter/submillimeter Array (ALMA) Band~2 receivers (67 - 116 GHz), whose commissioning…

星系天体物理 · 物理学 2026-05-18 Tom J. L. C. Bakx

Oxygen is the third most abundant element in the universe, but its chemistry in the interstellar medium is still not well understood. In order to critically examine the entire oxygen budget, we attempt here initially to estimate the…

太阳与恒星天体物理 · 物理学 2015-05-13 René Liseau , Kay Justtanont

Transmission spectra of H$_2$O+CO$_2$ mixtures have been recorded, at 296, 325 and 366 K, for various pressures and mixture compositions using two experimental setups. Their analysis enables to retrieve values of the 'continuum' absorption…

地球与行星天体物理 · 物理学 2019-05-01 Ha Tran , Martin Turbet , Simon Hanoufa , Xavier Landsheere , Pascale Chelin , Qiancheng Ma , Jean-Michel Hartmann

We present high-resolution optical spectroscopy of interstellar comet 3I/ATLAS (C/2025 N1) obtained with the High Dispersion Spectrograph mounted on the Subaru Telescope on UT 2026 January 7, when the comet was on its outbound trajectory at…

We report the results of a survey for HI 21-cm absorption at redshifts of z > 2.6 in a new sample of radio sources with the Green Bank and Giant Metrewave Radio Telescopes. From a total of 25 targets, we report zero detections in the 16 for…

星系天体物理 · 物理学 2020-09-02 S. J. Curran , R. W. Hunstead , H. M. Johnston , M. T. Whiting , E. M. Sadler , J. R. Allison , C. Bignell

We analyzed high resolution spectra of interstellar neutral carbon absorption toward $\lambda$ Ori, 1 Sco, and $\delta$ Sco that were obtained with the Goddard High Resolution Spectrograph on the Hubble Space Telescope. Several multiplets…

天体物理学 · 物理学 2009-11-06 S. R. Federman , J. Zsargo

We report a lambda > 1cm search for rotational molecular absorption towards quasars, now possible with the upgraded Australia Telescope Compact Array (ATCA). The targets were PKS 0201+113, PKS 0336-017 and Q 0537-286, where known damped…

天体物理学 · 物理学 2009-11-07 S. J. Curran , M. T. Murphy , J. K. Webb , Y. M. Pihlstroem