Chandra X-ray Observatory - HomeAbout The ChandraEducational MaterialsField GuidePhoto AlbumPress RoomResources
Chandra X-ray Observatory - HomeChandra Photo Album - You are here
ObservatoryImages by DateImages by CategorySky MapConstellationsSpecial FeaturesChandra Zoom-insImage HandoutsScale Bar ImagesTutorial Chandra Images & False Color Note on Cosmic DistanceCosmic Look Back TimeScale & DistanceScale & Angular MeasurementImage Use
Web Site ToolsVisit the Chandra ChroniclesEmail NewsletterSite MapNew & NoteworthyImage Use PolicyQuestions & AnswersGlossaryDownload Guide

TW Hydrae and HD 98800A:
Chandra Adds to Story of the Way We Were

TW Hydrae and HD 98800A
Credit: Spectra: NASA/CXC/RIT/J.Kastner et al.; Illustration: NASA/CXC/M.Weiss
JPEG (127 kb), Tiff (16.7 MB), PS (3.6 MB)

An artist's conception shows TW Hydrae (left) and HD 98800A (right), two young star systems that are both members of the TW Hydrae stellar association which formed about 10 million years ago. Chandra observations of their X-ray spectra revealed that, although the stars were both formed in the same region of space at the same time, they produce X-rays by different mechanisms.

The insets show portions of the X-ray spectra for each system. Of particular interest are the peaks labeled r, i, and f. These peaks, due to X-rays from neon atoms that have lost all but two of their ten orbital electrons, are sensitive indicators of the density and temperature in the hot, X-ray emitting gas in the star systems.

TW Hydrae and HD 98800A
The relative sizes of the peaks in TW Hydrae provide strong evidence that the matter is accreting onto the star from a circumstellar disk as shown in the illustration. X-rays are produced as matter is guided by the star's magnetic field onto one or more hot spots on the surface of the star.

In contrast, the spectrum of the binary star system HD 98800A revealed that its brightest star is producing X-rays much as the Sun does, from a hot upper atmosphere or corona. This indicates that any disk around these stars has been greatly diminished or destroyed in ten million years, perhaps by the ongoing formation of planets or by its companion stars.

Fast Facts for TW Hydrae:
Credit  Spectra: NASA/CXC/RIT/J.Kastner et al.; Illustration: NASA/CXC/M.Weiss
Coordinates (J2000)  RA 11h 01m 52.00s | Dec -34º 42' 16.00"
Constellation  Cetus
Observation Date  July 18, 2000
Observation Time  13.4 hours
Obs. ID  5
Instrument  ACIS/HETGS
Distance Estimate  About 190 light years from Earth
Release Date  May 26, 2003

Fast Facts for HD 98800A:
Credit  Spectra: NASA/CXC/RIT/J.Kastner et al.; Illustration: NASA/CXC/M.Weiss
Coordinates (J2000)  RA 11h 22m 05.30s | Dec -24º 46' 39.80"
Constellation  Crater
Observation Date  March 07, 2003
Observation Time  16.5 hours
Obs. ID  3728
Instrument  ACIS/HETGS
Distance Estimate  About 160 light years from Earth
Release Date  May 26, 2003

More Information on TW Hydrae and HD 98800A:
Press Room: TW Hydrae and HD 98800A Press Release
More Images of TW Hydrae and HD 98800A
TW Hydrae and HD 98800A Handout html | pdf
Powerpoint and PDF
More Information on Normal Stars & Star Clusters:
X-ray Astronomy Field Guide: Stars
Questions and Answers: Normal Stars & Star Clusters
Chandra Images: Normal Stars & Star Clusters


Chandra Images: '08 | ' 07 | ' 06 | ' 05 | ' 04 | ' 03 | ' 02 | ' 01 | ' 00 | ' 99 | Images by Category


separator line
CXC Home | Search | Help | Site Map | Image Use Policy | Privacy & Accessibility | Downloads & Plugins
Latest Images | New & Noteworthy | Multimedia | Flash Ecards | Glossary | Q&A | Guestbook


RSS Feed RSS Feed | Podcast Podcast | Blog Blog

[News by email: Chandra Digest]
[Contact us: cxcpub@cfa.harvard.edu]
NASA's Home Page Smithsonian's Home Page CXC Home Page Image Map for NASA's, Smithsonian and Chandra's Home Pages
Harvard-Smithsonian Center for Astrophysics
60 Garden Street, Cambridge, MA 02138 USA
Phone: 617.496.7941 Fax: 617.495.7356


Text Size:
normal font large font larger font
Chandra X-ray Center, Operated for NASA by the Smithsonian Astrophysical Observatory
This site was developed with funding from NASA under Contract NAS8-03060.
Revised: July 25, 2005