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Learn more about Bing search results hereStrong outflow of matter from a starOrganizing and summarizing search results for youAn inverse P Cygni profile is a feature in a spectrum that indicates a strong outflow of matter from a star. It is characterized by emission lines lying on the blue side of the absorption component.2 Sources
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inverse P Cygni profile with varying precision. Looking out for these inverse P Cygni profiles primarily allows us to find and identify molecular clouds that are undergoing infall motion.Low Mass Star Formation - Harvard University
The inverse P-Cygni profile of the observed water line generally indicates a contracting cloud. This profile is reproduced with a dynamical model of slow contraction from unstable quasi …
Understanding the P Cygni profile | Symposium - International ...
The P Cygni profile substructures caused by isolated reverse and forward shocks were calculated in a ‘line only’ approximation for a spherically symmetric, isothermal stellar wind. The …
- Author: Nadine Rons
- Publish Year: 1994
P Cygni line profile - Oxford Reference
4 days ago · The other parts of the shell produce the emission lines. Conversely, if material is falling on to the star, the absorption component can be redshifted relative to the emission …
Radiative transfer modeling of the observed line profiles in …
Jan 1, 2022 · Gorai et al. (2021) recently reported an inverse P-Cygni profile for the 1-0 transition of H 13 CO + in G31. Their analysis of this profile had suggested a clear indication of the …
- Author: Bratati Bhat, Prasanta Gorai, Prasanta Gorai, Suman Kumar Mondal, Sandip K. Chakrabarti, Ankan Das
- Publish Year: 2021
Schematic profile formation of a blended inverse P …
Schematic profile formation of a blended inverse P Cygni profile. (a) The supersonic (≈ 50 km/s) descending atmospheric layers produce a radiative emission centered on 0 km/s (blue curve). This...
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Inverse P Cygni profiles and their use in astronomical observations
Specifically, we would like to develop software that will take in an inverse P Cygni line profile of a molecular cloud undergoing infall motion, and give us back the infall rate that is required for …
We report the largest inverse P Cygni pro—le ever observed at this resolution: the depth of the Hb absorption com- ponent is nearly twice the height of the peak emission. Surprisingly, this …
[PDF] Inverse P Cygni profiles and their use in astronomical ...
Feb 9, 2017 · This research project would like to develop software that will take in an inverse P Cygni line profile of a molecular cloud undergoing infall motion, and give us back the infall rate …
Variability of Southern T Tauri Stars. I. The Continuum and the Hβ ...
Feb 10, 2001 · We report the largest inverse P Cygni profile ever observed at this resolution: the depth of the Hβ absorption component is nearly twice the height of the peak emission. …
Inverse P Cygni variability in the classical T Tauri star DR Tauri
Jul 21, 1997 · We have detected inverse P Cygni type profiles at HΔ in the spectrum of DR Tau. These profiles appeared and disappeared on a time-scale of hours.
Inverse P Cygni profiles and their use in astronomical observations
Feb 9, 2017 · We examine the effect of non-radial, magnetically-channeled wind outflow on P-Cygni line formation, using a Sobolev Exact Integration (SEI) approach for direct comparison …
Infall Model Parameters from Inverse P-Cygni Profiles
P-Cygni profiles exist in both CO and CH 3 CN for this source. As shown in Table 4, the two layer infall model is only able to reproduce the CO inverse P-Cygni profile if the rest velocity is...
[2201.10438] The sharp ALMA view of infall and outflow in the …
Jan 25, 2022 · The observations have revealed inverse P-Cygni profiles in CH3CN and H2CO toward the four sources embedded in the Main core, suggesting that all of them are …
[2107.04979] Radiative transfer modeling of the observed line …
Jul 11, 2021 · Abstract: An inverse P-Cygni profile of H13CO+ (1-0) in G31.41+0.31 was recently observed, which indicates the presence of an infalling gas envelope. Also, an outflow tracer, …
Spectroscopic Study of the Atmospheric Dynamics and Pulsation …
Feb 8, 2023 · The observation of the P Cygni and the inverse P Cygni profile indicate that expanding and infalling layers are simultaneously present in the stellar atmosphere, pointing …
Radiative transfer model to explain the observed line ... - NASA/ADS
Recently, a unique line profile of H 13 CO + has been observed in a high-mass star-forming region, G31.41+0.31. This particular type of profile is called the Inverse P-Cygni profile, …
Examples of inverse P Cygni profiles for different elements in S …
Download scientific diagram | Examples of inverse P Cygni profiles for different elements in S CrA SE. The wavelength (Å) and excitation potential (eV) are indicated.
Radiative transfer modeling to explain the observed Inverse P …
Here, in my presentation, I will present a detail radiative transfer model to reproduce the observed inverse P-Cygni profile and other emission features obtained. The evolution of stars is highly …
IRAS 16293–2422 Source B - SpringerLink
Nov 9, 2022 · The inverse P-Cygni profile is seen in the OCS, CH \(_3\) OH, HCOOCH \(_3\), and H \(_2\) CS lines toward the protostellar position. The situation illustrated in Fig. 7.12 b allows …
