appear in AJ Deep H I Survey of the Spiral Galaxy NGC 2403 Filippo Fraternali

نویسنده

  • Gustaaf van Moorsel
چکیده

High sensitivity H I observations of the nearby spiral galaxy NGC 2403 obtained with the VLA are presented and discussed. The properties of the extended, differentially rotating H I layer with its H I holes, spiral structure and outer warp are described. In addition, these new data reveal the presence of a faint, extended and kinematically anomalous component. This shows up in the H I line profiles as extended wings of emission towards the systemic velocity. In the central regions these wings are very broad (up to 150 km s) and indicate large deviations from circular motion. We have separated the anomalous gas component from the cold

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The HI halo of NGC 2403

The position-velocity diagram along the major axis of the Sc galaxy NGC 2403 shows the presence of gas with anomalous velocities (see Fig. 3 of the paper by Sancisi et al., this conference). This is the signature of an extended, slower rotating HI halo surrounding the thin disk (Schaap et al., 2000) We have isolated the ‘anomalous gas’ in NGC 2403 by fitting a Gaussian line profile to the thin ...

متن کامل

A low H i column density filament in NGC 2403 : signature of interaction or accretion

Observed H i accretion around nearby galaxies can only account for a fraction of the gas supply needed to sustain the currently observed star formation rates. It is possible that additional accretion happens in the form of low column density cold flows, as predicted by numerical simulations of galaxy formation. To contrain the presence and properties of such flows, we present deep H i observati...

متن کامل

2 00 1 A new , kinematically anomalous H I component in the spiral galaxy NGC 2403

We discuss new, high sensitivity H I observations of the spiral galaxy NGC 2403 which show extended emission at anomalous velocities with respect to the ‘cold’ disk. This ‘anomalous’ gas component (∼ 1/10 of the total H I mass) is probably located in the region of the halo and rotates more slowly (∼ 20−50 km s) than the gas in the disk. Moreover, it shows a distortion in the velocity field that...

متن کامل

Stationary Fluid Models for the Extra - Planar Gas in Spiral Galaxies

We show how to construct families of stationary hydrodynami-cal configurations that reproduce the observed vertical gradient of the rotation velocity of the extra-planar gas in spiral galaxies. We then present a simple model for the lagging halo of the spiral galaxy NGC 891, which is in agreement with the H i observations. Our method is based on well known properties of baroclinic solutions, an...

متن کامل

ar X iv : 0 70 5 . 40 34 v 1 [ as tr o - ph ] 2 8 M ay 2 00 7 The cold gaseous halo of NGC 891

We present H I observations of the edge-on galaxy NGC 891. These are among the deepest ever performed on an external galaxy. They reveal a huge gaseous halo, much more extended than seen previously and containing almost 30% of the H I. This H I halo shows structures on various scales. On one side, there is a filament extending (in projection) up to 22 kpc vertically from the disk. Small (MHI ∼ ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2002