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相关论文: The central part of the young open cluster NGC 638…

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By studying young open clusters, the mechanisms important for star formation over several Myr can be examined. For example, accretion rate as a function of rotational velocity can be investigated. Similarly, sequential star formation…

天体物理学 · 物理学 2009-01-06 E. Paunzen , M. Netopil , K. Zwintz

We present optical spectra of four intermediate mass candidate young stellar objects that have often been classified as Herbig Ae/Be stars. Typical Herbig Ae/Be emission features are not present in the spectra of these stars. Three of them,…

天体物理学 · 物理学 2009-11-07 P. Manoj , G. Maheswar , H. C. Bhatt

Using UBVRI Halpha CCD photometric observations and the archival NIR and X-ray data, we have carried out a multi-wavelength study of a young star cluster NGC 7419. An age of 22.5+/-3.0 Myr and a distance of 3230^{+330}_{-430} pc are derived…

天体物理学 · 物理学 2009-11-13 Himali Joshi , Brijesh Kumar , K. P. Singh , Ram Sagar , Saurabh Sharma , J. C. Pandey

The very young open cluster NGC 6383 centered on the O-star binary HD 159176 is an interesting place for studying the impact of early-type stars with strong radiation fields and powerful winds on the formation processes of low-mass stars.…

太阳与恒星天体物理 · 物理学 2015-05-14 G. Rauw , J. Manfroid , M. De Becker

This study focuses on determining the characteristics of the young open cluster NGC 6383. To achieve this, the HDBSCAN clustering algorithm is utilized to identify potential cluster members based on proper motions and parallaxes from Gaia…

星系天体物理 · 物理学 2024-10-17 L. M. Pulgar-Escobar , N. A. Henríquez-Salgado

Context. Stellar physical properties of star clusters are poorly known. Aims. Our goals are to perform a spectrophotometric study of the B star population in open clusters to derive accurate stellar parameters, search for the presence of…

太阳与恒星天体物理 · 物理学 2018-02-21 Y. Aidelman , L. S. Cidale , J. Zorec , J. A. Panei

The interstellar extinction law in twenty open star clusters namely Berkeley 7, Collinder 69, Hogg 10, NGC 2362, Czernik 43, NGC 6530, NGC 6871, Bochum 10, Haffner 18, IC 4996, NGC 2384, NGC 6193, NGC 6618, NGC 7160, Collinder 232, Haffner…

星系天体物理 · 物理学 2017-12-27 Geeta Rangwal , R. K. S. Yadav , Alok Durgapal , D. Bisht

The number and the nature of emission line stars in the young open cluster NGC6611 is still the object of debates. Due to the presence of a strong and variable nebulosity in the cluster, the number of emission line stars is highly depending…

The extinction law and the variation of colour excess with position, luminosity as well as spectral class in young open star clusters NGC 663, NGC869, NGC 884, NGC 1502, NGC 1893, NGC 2244, NGC 2264, NGC 6611, Tr 14, Tr 15,Tr 16, Coll 228,…

天体物理学 · 物理学 2009-11-06 R. K. S. Yadav , Ram Sagar

Hidden from optical view in the starburst region of the dwarf galaxy NGC 5253 lies an intense radio source with an unusual spectrum which could be interpreted variously as nebular gas ionized by a young stellar cluster or nonthermal…

天体物理学 · 物理学 2009-11-06 Varoujan Gorjian , Jean L. Turner , Sara C. Beck

We present uvby-beta CCD photometry of the field of the open cluster NGC 1893. Our photometry is deep enough to cover the complete main sequence B spectral type. We identify ~50 very likely members of the cluster down to spectral type…

天体物理学 · 物理学 2009-11-06 A. Marco , I. Negueruela , G. Bernabeu

The spectral and reddening properties of 211 highly reddened proper motion members with $V < 15$ mag in 6 young galactic star clusters are investigated using low resolution spectroscopic, broad-band $UBVRIJHK$ and mid-IR data. We report…

天体物理学 · 物理学 2009-11-10 Brijesh Kumar , Ram Sagar , B. B. Sanwal , M. S. Bessell

We present new near-infrared spectroscopic observations of the outer edges of the young stellar cluster around the supermassive black hole at the Galactic center. The observations show a break in the surface-density profile of young stars…

星系天体物理 · 物理学 2015-08-06 Morten N. Støstad , Tuan Do , Norm Murray , Jessica R. Lu , Sylvana Yelda , Andrea M. Ghez

Searches for planetary transits carried out in open and globular clusters have yielded to date only a handful of weak, unconfirmed candidates. These results have been interpreted either as being insignificant, or as evidence that the…

地球与行星天体物理 · 物理学 2015-06-04 V. Nascimbeni , L. R. Bedin , G. Piotto , F. De Marchi , R. M. Rich

A search for pulsating pre-main sequence (PMS) stars was performed in the young open cluster NGC 6383 using CCD time series photometry in Johnson B & V filters. With an age of only ~1.7 million years all cluster members later than spectral…

天体物理学 · 物理学 2009-11-10 K. Zwintz , M. Marconi , P. Reegen , W. W. Weiss

We analyze spectra of 44 emission line stars detected in a low resolution optical spectroscopic survey of the galactic open cluster NGC 6871. The survey of 1217 stars is complete to V = 14.9 and includes stars with V < 16.5 between the zero…

天体物理学 · 物理学 2009-11-07 Zoltan Balog , Scott J. Kenyon

The full stellar population of NGC 6334, one of the most spectacular regions of massive star formation in the nearby Galaxy, have not been well-sampled in past studies. We analyze here a mosaic of two Chandra X-ray Observatory images of the…

星系天体物理 · 物理学 2015-05-13 Eric D. Feigelson , Amanda L. Martin , Collin J. McNeill , Patrick S. Broos , Gordon P. Garmire

Relying on U,B imagery at the Italian Telescopio Nazionale Galileo (TNG), we report here the discovery of a sample of 13 new UV-bright post-HB candidate stars in the field of the galactic open cluster NGC 6791. Owing to its super-solar…

天体物理学 · 物理学 2016-08-30 L. M. Buson , E. Bertone , A. Buzzoni , G. Carraro

We investigate the star cluster population in the outer parts of the starburst galaxy NGC 5253 using archive images taken with the Hubble Space Telescope's Advanced Camera for Surveys. Based on the F415W, F555W, and F814W photometry ages…

宇宙学与河外天体物理 · 物理学 2015-06-04 D. Harbeck , J. Gallagher , D. Crnojević

Ultraviolet, optical and near infrared images of the nearby (D ~ 5.5 Mpc) SBm galaxy NGC 1311, obtained with the Hubble Space Telescope, reveal a small population of 13 candidate star clusters. We identify candidate star clusters based on a…

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