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相关论文: Origin of the PN molecule in star-forming regions:…

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We present multi-transition observations of PN towards a sample of nine massive dense cores in different evolutionary stages. Using transitions with different excitation conditions, we have found for the first time that the excitation…

星系天体物理 · 物理学 2018-03-14 C. Mininni , F. Fontani , V. M. Rivilla , M. T. Beltrán , P. Caselli , A. Vasyunin

Phosphorus (P) is one of the important elements for the formation of life and plays a crucial role in several biochemical processes. Recent spectral line surveys have confirmed the existence of P-bearing molecules, especially PN and PO, in…

星系天体物理 · 物理学 2023-12-25 Arijit Manna , Sabyasachi Pal

Phosphorus is a crucial element for the development of life, but so far P-bearing molecules have been detected only in a few astrophysical objects, hence its interstellar chemistry is almost totally unknown. Here we show new detections of…

星系天体物理 · 物理学 2016-05-25 F. Fontani , V. M. Rivilla , P. Caselli , A. Vasyunin , Aina Palau

As part of the Large Program ASAI (Astrochemical Surveys At IRAM), we have used the IRAM 30m telescope to lead a systematic search for the emission of rotational transitions of P-bearing species between 80 and 350 GHz towards L1157-B1, a…

Phosphorus (P) is a crucial element for life given its central role in several biomolecules. P-bearing molecules have been discovered in different regions of the Milky Way, but not yet towards an extragalactic environment. We have searched…

The astrochemistry of the important biogenic element phosphorus (P) is still poorly understood, but observational evidence indicates that P-bearing molecules are likely associated with shocks. We study P-bearing molecules, as well as some…

Phosphorus is a necessary element for life on Earth, but at present we have limited constraints on its chemistry in star- and planet-forming regions: to date, phosphorus carriers have only been detected towards a few low-mass protostars.…

星系天体物理 · 物理学 2022-08-17 Serena Wurmser , Jennifer B. Bergner

For decades, the detection of phosphorus-bearing molecules in the interstellar medium was restricted to high-mass star-forming regions (as e.g. SgrB2 and Orion KL) and the circumstellar envelopes of evolved stars. However, recent…

星系天体物理 · 物理学 2018-08-08 Izaskun Jimenez-Serra , Serena Viti , David Quenard , Jonathan Holdship

Phosphorus is a key ingredient in terrestrial biochemistry, but is rarely observed in the molecular ISM and therefore little is known about how it is inherited during the star and planet formation sequence. We present observations of the…

太阳与恒星天体物理 · 物理学 2019-11-06 Jennifer B. Bergner , Karin I. Oberg , Salma Walker , Viviana V. Guzman , Thomas S. Rice , Edwin A. Bergin

We present spectral line mapping observations toward four massive star-forming regions (Cepheus A, DR21S, S76E and G34.26+0.15), with the IRAM 30 meter telescope at 2 mm and 3 mm bands. Totally 396 spectral lines from 51 molecules, one…

星系天体物理 · 物理学 2017-01-18 Shanghuo Li , Junzhi Wang , Zhi-Yu Zhang , Min Fang , Juan Li , Jiang- shui Zhang , Junhui Fan , Qingfeng Zhu , Fei Li

Phosphorus is a crucial element in biochemistry, especially the P-O bond, which is key for the formation of the backbone of the deoxyribonucleic acid. So far, PO has only been detected towards the envelope of evolved stars, and never…

星系天体物理 · 物理学 2016-08-17 V. M. Rivilla , F. Fontani , M. T. Beltrán , A. Vasyunin , P. Caselli , J. Martín-Pintado , R. Cesaroni

Phosphorus is a key element that plays an essential role in biological processes important for living organisms on Earth. The origin and connection of phosphorus-bearing molecules to early Solar system objects and star-forming molecular…

We present medium-resolution K-band long-slit spectroscopy of 29 true, likely, possible and candidate Galactic Plane planetary nebulae (PNe) from the UWISH2 survey - many of which have only been recently discovered. These objects are bright…

太阳与恒星天体物理 · 物理学 2018-08-09 A. M. Jones , T. M. Gledhill , D. Froebrich , M. D. Smith

We present medium-resolution (R~700) near-infrared (lambda = 1 - 2.5 micron) spectra of a sample of planetary nebulae (PNe). A narrow slit was used which sampled discrete locations within the nebulae; observations were obtained at one or…

天体物理学 · 物理学 2009-10-31 Joseph L. Hora , William B. Latter , Lynne K. Deutsch

We report the first detections of OH$^+$ emission in planetary nebulae (PNe). As part of an imaging and spectroscopy survey of 11 PNe in the far-IR using the PACS and SPIRE instruments aboard the Herschel Space Observatory, we performed a…

The present survey represents a continuation of our study of high mass star forming regions in the lines of deuterated molecules, the first results of which were published in Trofimova et al. (2020). This paper presents the results of…

星系天体物理 · 物理学 2024-09-17 E. Trofimova , I. Zinchenko , P. Zemlyanukha , M. Thomasson

Protostellar outflows are considered a signpost of star formation. These outflows can cause shocks in the molecular gas and are typically traced by the line wings of certain molecules. HNCO (4--3) has been regarded as a shock tracer because…

星系天体物理 · 物理学 2023-06-07 Jinjin Xie , Juan Li , Junzhi Wang , Shu Liu , Kai Yang , Donghui Quan , Siqi Zheng , Yuqiang Li , Jingwen Wu , Yan Duan , Di Li

(Abridged) Complex organic molecules (COMs) are commonly detected in and near star-forming regions. However, the dominant process in the release of these COMs from the icy grains - where they predominately form - to the gas phase is still…

太阳与恒星天体物理 · 物理学 2021-11-24 S. J. van der Walt , L. E. Kristensen , J. K. Jørgensen , H. Calcutt , S. Manigand , M. el Akel , R. T. Garrod , K. Qiu

We have searched the entire ROSAT archive for useful observations to study X-ray emission from Galactic planetary nebulae (PNs). The search yields a sample of 63 PNs, which we call the ROSAT PN sample. About 20-25% of this sample show X-ray…

天体物理学 · 物理学 2009-10-31 Martin A. Guerrero , You-Hua Chu , Robert A. Gruendl

The reactions of the low-lying metastable states of atomic phosphorus, P($^2$D) and P($^2$P), with H$_{2}$O and H$_{2}$ were studied by the pulsed laser photolysis at 248 nm of PCl$_{3}$ , combined with laser induced fluorescence detection…

太阳与恒星天体物理 · 物理学 2022-06-29 Kevin M. Douglas , David Gobrecht , John M. C. Plane
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