Emission nebulae

Results: 34



#Item
1ASTROPHYSICS SEMINAR Tuesday, 10 February 2009 at 14:00 Pulsar Wind Nebulae and Polarized Gamma-Ray Emission from the Crab

ASTROPHYSICS SEMINAR Tuesday, 10 February 2009 at 14:00 Pulsar Wind Nebulae and Polarized Gamma-Ray Emission from the Crab

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Source URL: isdc.unige.ch

Language: English - Date: 2009-08-28 04:49:22
    2The Interstellar Medium (ISM) • Observations: – gas and dust fills the space between the stars  ISM • In the optical – Emission and Reflection nebulae You will meet a

    The Interstellar Medium (ISM) • Observations: – gas and dust fills the space between the stars  ISM • In the optical – Emission and Reflection nebulae You will meet a

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    Source URL: hyperion2.cc.uregina.ca

    Language: English - Date: 2015-04-10 15:56:30
    3Monte Carlo simulations of X-ray reflection nebulae in the Galactic Center region for future high-resolution imaging spectroscopy Hirokazu Odaka1, Shin Watanabe1, Tadayuki Takahashi1, Felix Aharonian2,3, Dmitry Khangulya

    Monte Carlo simulations of X-ray reflection nebulae in the Galactic Center region for future high-resolution imaging spectroscopy Hirokazu Odaka1, Shin Watanabe1, Tadayuki Takahashi1, Felix Aharonian2,3, Dmitry Khangulya

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    Source URL: www.sron.nl

    Language: English - Date: 2010-04-01 07:35:44
    4Uranometria’s Dark Nebulae Database This atlas contains 367 dark nebulae, which are drawn to scale with a dashed outline if larger than 10′. Objects smaller than 10′ are drawn as dashed-line square boxes in

    Uranometria’s Dark Nebulae Database This atlas contains 367 dark nebulae, which are drawn to scale with a dashed outline if larger than 10′. Objects smaller than 10′ are drawn as dashed-line square boxes in

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    Source URL: willbell.com

    Language: English - Date: 2008-10-21 20:05:56
    5UranometriaDeep Sky Field Guide Planetary Nebulae will usually appear to “blink” as the stars are dimmed, and the nebula retains it brightness. There are a few planetaries that have weak [OIII] emission (a br

    UranometriaDeep Sky Field Guide Planetary Nebulae will usually appear to “blink” as the stars are dimmed, and the nebula retains it brightness. There are a few planetaries that have weak [OIII] emission (a br

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    Source URL: willbell.com

    Language: English - Date: 2008-10-30 00:00:21
    6Uranometria’s Bright Nebulae Database We draw to scale 377 bright nebulae with a solid outline if larger than 10′. Objects smaller than 10′ are drawn as solid-line square boxes in two sizes (10′ to 5′ an

    Uranometria’s Bright Nebulae Database We draw to scale 377 bright nebulae with a solid outline if larger than 10′. Objects smaller than 10′ are drawn as solid-line square boxes in two sizes (10′ to 5′ an

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    Source URL: willbell.com

    Language: English - Date: 2008-10-21 20:01:19
    7Publ. Astron. Soc. Aust., 1998, 15, 123–7 . Hα Emission from Point Sources in the Magellanic Clouds D. H. Morgan Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UK

    Publ. Astron. Soc. Aust., 1998, 15, 123–7 . Hα Emission from Point Sources in the Magellanic Clouds D. H. Morgan Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UK

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    Source URL: www.roe.ac.uk

    Language: English - Date: 2000-04-07 11:28:52
    8Sagittarius: Stellar Nurseries -- Teacher Page Purpose of the Sagittarius Activity: This activity will allow students the opportunity to attempt to solve a problem using real astronomical equipment and data analysis. Usi

    Sagittarius: Stellar Nurseries -- Teacher Page Purpose of the Sagittarius Activity: This activity will allow students the opportunity to attempt to solve a problem using real astronomical equipment and data analysis. Usi

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    Source URL: www.gb.nrao.edu

    Language: English - Date: 2012-08-03 12:32:27
    9H II Nuclei in Nearby Galaxies Wendy Hawley Journal Club “Properties of H II Regions in the Centers of Nearby Galaxies” (Ho, L.C., Filippenko, A.V., & Sargent, W.L.W. 1997, ApJ 487, 579)

    H II Nuclei in Nearby Galaxies Wendy Hawley Journal Club “Properties of H II Regions in the Centers of Nearby Galaxies” (Ho, L.C., Filippenko, A.V., & Sargent, W.L.W. 1997, ApJ 487, 579)

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    Source URL: www.asu.edu

    Language: English - Date: 2007-02-23 19:29:11
    10The Astronomical Journal, 124:3336–3339, 2002 December # 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A. MEASUREMENTS OF [O i] 6300/H LINE INTENSITY RATIOS FOR FOUR O STAR H ii REGIONS

    The Astronomical Journal, 124:3336–3339, 2002 December # 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A. MEASUREMENTS OF [O i] 6300/H LINE INTENSITY RATIOS FOR FOUR O STAR H ii REGIONS

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    Source URL: www.astro.wisc.edu

    Language: English - Date: 2007-02-15 11:52:04