About: Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive

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scholarly article

Attributes	Values
rdf:type	Item
description	wetenschappelijk artikel (nl) գիտական հոդված (hy) scholarly article (en) наукова стаття, опублікована в лютому 2014 (uk) im Februar 2014 veröffentlichter wissenschaftlicher Artikel (de)
publication date	wds:Q58920527-322664B9-0069-4190-895C-92058A271FEB
publication date	2014-02-05 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q58920527-9755BF05-14C0-4394-9F50-381048C611AC
language of work or name	English
cites work	wds:Q58920527-0E13A1CC-7D3B-4A87-A024-972693DD6AAE wds:Q58920527-0E60EB04-EE3E-4908-A9D3-763FDF16E2AB wds:Q58920527-1406C038-FA0B-400C-86E9-47704605870D wds:Q58920527-1530084C-C982-41BD-8748-8FDC29C88952 wds:Q58920527-1B5FA7C3-9987-482E-B436-096E5488E4DE wds:Q58920527-2CEB144E-B3B3-47AE-B1D1-E24EB5769BB8 wds:Q58920527-30620843-565F-43CA-B816-399A4D7D8C9F wds:Q58920527-3794C200-CAF6-451B-B802-BB2DFD12891A wds:Q58920527-57F8BEDE-10C4-479C-92BF-7D964FB7D370 wds:Q58920527-5B3DC71A-5F6A-4A95-A9E2-9AEA7BC602EA wds:Q58920527-6226AAC2-5FF2-4344-927E-B9221A18A2CE wds:Q58920527-6710D612-4A76-45C9-991F-1B76B905A9E7 wds:Q58920527-70F16FBA-AF16-4988-82E7-F037D97483E7 wds:Q58920527-93E49929-D727-4FB9-8580-945C64C82FE6 wds:Q58920527-98D80CA1-84F8-40E5-B24F-98BC7EF73801 wds:Q58920527-9D283FC6-B76C-4EBF-B86C-0956715CAF1A wds:Q58920527-A3ECB4F3-55A2-463A-8E6F-D7A879FDDB55 wds:Q58920527-BC8D91B1-2C98-4D79-A2A8-626636F1412E wds:Q58920527-BDDA075E-930C-496B-BA1A-49AA910DCA11 wds:Q58920527-D8A8759D-74E6-49E3-A3BC-7FC891D05D8D wds:Q58920527-D902BFD7-C15D-4B5D-855C-D26563C9DBEC wds:Q58920527-E7BCB9A3-F680-4C1A-ADB8-EB16E288BEA1 wds:Q58920527-EF2714F0-B287-4608-BD6E-ECA7B00FADA6 wds:Q58920527-F1B14AB7-5D2D-4C6B-9D61-9AD1F8655BB1 wds:Q58920527-FE7043B6-5D2D-49C8-8F13-70D9B8A188E8
cites work	Stellar and wind parameters of Galactic O-stars. The influence of line-blocking/blanketing The Chemical Composition of the Sun A new calibration of stellar parameters of Galactic O stars High resolution X-ray spectroscopy ofζPuppis with the XMM-Newton reflection grating spectrometer On the origin of the O and B-type stars with high velocities. II. Runaway stars and pulsars ejected from the nearby young stellar groups A Grid of Non‐LTE Line‐blanketed Model Atmospheres of O‐Type Stars ι Orionis—Evidence for a Capture Origin Binary Spectral analysis of early-type stars using a genetic algorithm based fitting method Chandra spectroscopy of the hot star β Crucis and the discovery of a pre-main-sequence companion Constraints on porosity and mass loss in O-star winds from the modeling of X-ray emission line profile shapes A generalized porosity formalism for isotropic and anisotropic effective opacity and its effects on X-ray line attenuation in clumped O star winds A magnetic confinement versus rotation classification of massive-star magnetospheres Properties of Galactic early-type O-supergiants An introduction to the Chandra Carina complex project Measurements and Analysis of Helium‐like Triplet Ratios in the X‐Ray Spectra of O‐Type Stars Wind signatures in the X-ray emission-line profiles of the late-O supergiant Orionis Quantitative studies of the optical and UV spectra of Galactic early B supergiants XMM��Newtonobservations of the massive colliding wind binary and non-thermal radio emitter Cyg��OB2��#8A [O6If + O5.5III(f)] Chandra X-ray spectroscopy of the very early O supergiant HD 93129A: constraints on wind shocks and the mass-loss rate Hot and cool: two emission-line stars with constrasting behaviours in the same XMM-Newtonfield Modeling broadband X-ray absorption of massive star winds The non-thermal radio emitter HD 93250 resolved by long baseline interferometry ζ Orionis A is a Double Star Evidence for the Importance of Resonance Scattering in X‐Ray Emission Line Profiles of the O Star ζ Puppis Resolving OB Systems in the Carina Nebula with the Hubble Space Telescope Fine Guidance Sensor
author name string	wds:Q58920527-2B494AF2-5C18-4EEA-80EF-03B2598FAE21 wds:Q58920527-A6D8852A-2ED1-4957-BC5E-84365F474232 wds:Q58920527-B39507CF-E2BE-4E4E-9A72-9B482832CA7B wds:Q58920527-BFBDF157-353D-43D7-B19E-1776F5C01C80 wds:Q58920527-D1A23D29-6059-4E69-B547-4D2C5FE75A74 wds:Q58920527-E51274BB-E352-44D6-B621-298F733C245C wds:Q58920527-EF49DDEA-BA49-4699-ADC3-AA4361DE38F8
author name string	Stanley P. Owocki David H. Cohen Alex W. Fullerton Jon O. Sundqvist Maurice A. Leutenegger Emma E. Wollman Janos Zsargó
rdfs:label	Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive (en) Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive (nl)
skos:prefLabel	Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive (en) Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive (nl)
name	Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive (en) Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive (nl)
title	wds:Q58920527-A7A8DF9F-208F-4988-B7DE-0F6C447F4654
title	Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive (en)
page(s)	wds:Q58920527-A31F6CE8-7BBD-4791-B442-D2C5BE5E2955
page(s)	908–923
Internet Archive ID	wds:Q58920527-75F0E1C0-3EA3-4FE9-A6F5-CDD511CAC19D
Internet Archive ID	arxiv-1401.7995
instance of	wds:Q58920527-37235D89-E6D6-4EFB-B07D-5F41DF9F4480
instance of	scholarly article
published in	wds:Q58920527-F8652EDE-E48E-43CD-A8FF-6523C32E693F
published in	Monthly Notices of the Royal Astronomical Society
issue	wds:Q58920527-2479A534-6512-4652-9FD2-CB2BA3034FF3
volume	wds:Q58920527-B5550F44-2383-460F-80A6-6654EF65FA40
issue	1
volume	439
number of pages	wds:Q58920527-72B688A8-3358-4221-86C5-E2D416FF3013
number of pages	16 (xsd:decimal)
DOI	wds:Q58920527-EAF24C54-0580-4A07-BBF3-E48B5819E7CF
DOI	http://dx.doi.org/10.1093/MNRAS/STU008
DOI	10.1093/MNRAS/STU008
arXiv ID	wds:Q58920527-AB74FDC1-EEA1-4EF8-ABDE-91FCF75ADF04

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