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相关论文: Spectral Properties and Variability of BIS objects

200 篇论文

We present a new catalog of 11,209 O-rich AGB stars and 7172 C-rich AGB stars in our Galaxy identifying more AGB stars in the bulge component and considering more visual carbon stars. For each object, we cross-identify the IRAS, AKARI, MSX,…

太阳与恒星天体物理 · 物理学 2021-10-20 Kyung-Won Suh

We present a catalog of 110 variable stars within ~1' of Sgr A* based on image subtraction of near-infrared (H and K) photometry. Our images were obtained over 133 nights from 2000--2002 in H-band and over 134 nights from 2001--2002 in…

天体物理学 · 物理学 2007-08-06 Molly S. Peeples , K. Z. Stanek , D. L. DePoy

We analyze five epochs of Spitzer Space Telescope/Infrared Array Camera (IRAC) observations of the nearby spiral galaxy M33. Each epoch covered nearly a square degree at 3.6, 4.5, and 8.0 microns. The point source catalog from the full…

We present a compilation and study of DENIS, 2MASS, ISOGAL, MSX and IRAS 1--25 micron photometry for a sample of 441 late-type stars in the inner Galaxy, which we previously searched for 86 GHz SiO maser emission (Messineo et al.2002). The…

天体物理学 · 物理学 2009-11-10 M. Messineo , H. J. Habing , K. M. Menten , A. Omont , L. O. Sjouwerman

Near-infrared, JHKL, photometry of 239 Galactic carbon-rich variable stars is presented and discussed. From these and published data the stars were classified as Mira or non-Mira variables and amplitudes and pulsation periods, ranging from…

天体物理学 · 物理学 2009-11-11 Patricia A. Whitelock , Michael W. Feast , Freddy Marang , M. A. T. Groenewegen

We report new results of our search for rare, cool carbon stars located at large distances from the galactic plane. Eighteen new C stars were discovered. Six are remarkable by showing the two peculiarities of a strong infrared excess at 12…

天体物理学 · 物理学 2010-04-21 Nicolas Mauron

We have identified 139 cool carbon stars in the near-infrared spectro-photometric survey of the InfraRed Telescope in Space (IRTS) from the conspicuous presence of molecular absorption bands at 1.8, 3.1 and 3.8 microns. Among them 14 are…

天体物理学 · 物理学 2007-05-23 T. Le Bertre , M. Tanaka , I. Yamamura , H. Murakami , D. J. MacConnell

A high-resolution ($\sim$45000), high signal-to-noise ($>$100) K-band spectral atlas of massive stars is presented. It includes 81 stars consisting of known optical standards, spanning spectral and luminosity subclasses from O2 to O9, and…

太阳与恒星天体物理 · 物理学 2026-05-01 V. M. Kalari , W. D. Vacca

We present a study of ISOGAL sources in the "intermediate" galactic bulge ($|$$l$$|$ $<$ 2$^\circ$, $|$$b$$|$ $\sim$ 1$^\circ$--4$^\circ$), observed by ISOCAM at 7 and 15 $\mu m$. In combination with near-infrared (I, J, K$_{\rm s}$) data…

天体物理学 · 物理学 2009-11-07 D. K. Ojha , A. Omont , F. Schuller , G. Simon , S. Ganesh , M. Schultheis

New multi-epoch, mid-infrared (8-13 microns) spectrophotometric observations are presented for 30~late-type stars. The observations were collected over a four year period (1994-1997), permitting an investigation of the mid-infrared spectral…

天体物理学 · 物理学 2009-10-30 J. D. Monnier , T. R. Geballe , W. C. Danchi

We have searched for near-infrared stellar counterparts of IRAS point sources in the Large Magellanic Cloud (LMC), in J and K-bands. This resulted in the detection of 21 counterparts, of which 19 are new discoveries. Using colour-magnitude…

We present ISO photometric and spectroscopic observations of a sample of 57 bright Asymptotic Giant Branch stars and red supergiants in the Large Magellanic Cloud, selected on the basis of IRAS colours indicative of high mass-loss rates.…

It is the purpose of this paper to rediscuss the circumstellar properties of S stars and to put these properties in perspective with our current understanding of the evolutionary status of S stars, in particular the intrinsic/extrinsic…

天体物理学 · 物理学 2009-10-30 A. Jorissen , G. R. Knapp

The identification of IRAS sources with Faint Markarian galaxies on the base of the Second Byurakan Survey were made. It is shown that about 30% of SBS galaxies are also IRAS sources.The list of newly identified objects are presented.

天体物理学 · 物理学 2007-05-23 V. T. Ayvazyan

An analysis of low resolution spectra and infared data of 29 ISOGAL-DENIS sources with mid-IR excess is presented. Eight ISOGAL sources from our sample with 7-15 micron excess are found to be B and A-type stars, some of them with emission…

天体物理学 · 物理学 2009-11-07 M. Schultheis , M. Parthasarathy , A. Omont , M. Cohen , S. Ganesh , F. Sevre , G. Simon

We have obtained high resolution (R = 10,000) K-band spectra of candidate young massive stars deeply embedded in (ultra-) compact HII regions (UCHIIs). In these clusters, three types of objects are identified. The first type (38 objects)…

天体物理学 · 物理学 2009-11-11 A. Bik , L. Kaper , M. M. Hanson , M. Smits

Using infrared photometric data extracted from the 2MASS, IRAS and MSX databases, 142 suspected young stellar objects (YSOs) are selected from about 2 million stars in the Camelopardalis segment of the Milky Way limited by Galactic…

天体物理学 · 物理学 2009-06-25 V. Straizys , V. Laugalys

IRAS 19312+1950 is a peculiar object that has eluded firm characterization since its discovery, with combined maser properties similar to an evolved star and a young stellar object (YSO). To help determine its true nature, we obtained…

We analyze the differences in infrared circumstellar dust emission between oxygen rich Mira and non-Mira stars, and find that they are statistically significant. In particular, we find that these stars segregate in the K-[12] vs. [12]-[25]…

天体物理学 · 物理学 2009-11-06 M. Marengo , Z. Ivezic , G. R. Knapp

Our understanding of large amplitude pulsating stars and their status in stellar evolution is briefly reviewed. The paper then describes the near-infrared light curves of various asymptotic giant branch stars, concentrating on possible…

天体物理学 · 物理学 2007-05-23 Patricia A. Whitelock